The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a high degree of luminosity, appearing nearly spherical and concentrated. This suggests a dense stellar population and potentially an active galactic nucleus, although further spectroscopic data would be required to confirm the latter. The galaxy's luminosity gradually decreases towards the outer edges, with a subtle flattening visible along one axis, indicating a possible transition towards a more lenticular morphology. Faint, diffuse light extends beyond the main body of the galaxy, forming a halo-like structure. There is no obvious evidence of spiral arms or prominent dust lanes, further supporting a classification as an elliptical or lenticular galaxy. The color appears to be relatively uniform throughout, with a yellowish hue indicative of an older stellar population, and comparatively low levels of current star formation. There are indications of only minor gravitational disturbances.
