The galaxy presents as a smooth, centrally concentrated object with a mostly elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The central bulge region is bright and well-defined, suggesting a high concentration of stars, possibly an older stellar population. Surrounding the bulge is a more diffuse halo or disk. The disk appears somewhat asymmetric, with a slight elongation or distortion on one side, potentially indicating a past minor interaction or disturbance. The overall color appears relatively uniform across the galaxy, with subtle variations, suggesting ongoing, but not intense, star formation within the disk. There are some indications that the galaxy could be actively forming stars, though at a low rate. There appears to be little evidence of a major ongoing merger.
