The galaxy appears to be relatively compact and luminous, with an approximate diameter of 9 kpc. The light profile suggests a fairly smooth distribution, indicating an elliptical or lenticular morphology. The central region shows a strong concentration of light, appearing yellowish, possibly indicative of an older stellar population. Fainter, diffuse light extends outwards from the core. A hint of bluer light is observed in the outer regions, suggestive of some degree of recent star formation. There may be some tidal features or minor disturbances present, however, the current resolution makes this difficult to confirm. There is a general lack of spiral arms or any clear disk structure. The galaxy appears to be isolated, without any obvious signs of ongoing or recent interactions with neighboring galaxies.
