The galaxy presents as a somewhat smooth, centrally concentrated light distribution. It exhibits a roughly circular morphology, with a subtle elongation or deviation from a perfect circle. The core region appears bright and compact, suggesting a high stellar density or the presence of an active galactic nucleus (AGN), although the resolution does not permit definitive identification.

The galaxy displays a color gradient, with the central regions appearing slightly more yellow or red-shifted than the outer regions, which have a bluer hue. This may indicate a younger stellar population in the outer disk or ongoing star formation. The absence of prominent spiral arms or strong dust lanes suggests that the galaxy is either an elliptical or a relatively face-on spiral galaxy with smooth arm structure. There is potentially minor disturbance in the galaxy, but is most likely a single component galaxy.

Overall, the galaxy appears to be a relatively undisturbed system with moderate star formation activity and a substantial central mass concentration. Further spectroscopic and high-resolution imaging would be necessary to confirm its morphological type and detailed physical properties.
