The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated luminosity profile. It has a noticeable bulge, with a flattened disc component oriented at an angle relative to our line of sight. The color is somewhat redder in the central bulge region, potentially indicating an older stellar population. Moving outward, the disk exhibits bluer hues, suggestive of ongoing or recent star formation, although this is not very pronounced. The galaxy displays a moderate degree of ellipticity, with its major axis extending further than its minor axis. There are no significant tidal features or other obvious signs of a major merger event. The overall structure is relatively undisturbed.
