The galaxy appears to be an elliptical or lenticular type, with a somewhat cigar-shaped morphology. The central bulge exhibits a smooth, concentrated distribution of light, appearing yellow-white suggesting an older stellar population. This bright central region transitions into a more diffuse outer halo. The colors shift subtly from yellow-white to a bluer hue, most notably on the upper and lower edge of the galaxy. This implies the presence of a younger, bluer stellar population extending outwards. Faint wisps or features are possibly present but the image resolution makes them hard to discern. There are suggestions of minor tidal disturbances or asymmetries in the outskirts, which may be indicative of past interactions or mergers, but these are not distinctly pronounced.
