The galaxy appears as an elliptical structure exhibiting a smooth morphology, as suggested by the relatively high "smooth or featured smooth" fraction reported. Its shape is elongated, tending toward cigar-shaped. There are no apparent signs of a major merger or significant tidal disturbances, though subtle asymmetries might indicate minor gravitational interactions or internal processes.

There is a color gradient across the galaxy, with a reddish central region which could be the result of older stellar populations and/or dust obscuration. The outer regions appear bluer, possibly indicating the presence of younger, hotter stars. The galaxy shows no clear spiral arms, bars, or prominent dust lanes, which is consistent with an elliptical morphology.
