The galaxy presents a relatively smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that dominates the overall luminosity. The surrounding disk appears somewhat diffuse and lacks clearly defined spiral arm structures. There is a slight flattening visible, suggesting it is not perfectly spherical. Color gradients are subtle, with the core appearing more yellow and potentially indicative of an older stellar population, while the outer regions show a hint of bluer hues possibly tracing younger stars or regions of ongoing star formation, although the image quality is not high enough to confirm. There does not appear to be any major merging or tidal disruption, although the disk may have experienced minor disturbances.
