The galaxy presents as a somewhat diffuse object, exhibiting a generally elliptical morphology. The central region displays a concentrated luminosity gradient. There are distinct features of moderate disturbance in the galaxy's structure, perhaps indicative of tidal interactions or internal processes. A faint, yet extended halo surrounds the bright central region, which may suggest recent or ongoing star formation, as suggested by a blue-ish hue. There appears to be a lack of significant dust lanes or prominent spiral arm structure. The galaxy appears to be relatively isolated in this field of view. Overall, the morphology seems to be somewhere between an elliptical and a disturbed spiral galaxy. There are some faint redder areas possibly indicative of older star populations, which might be indicative of an elliptical galaxy.
