The galaxy exhibits a generally smooth morphology with a slight elongation, appearing more lenticular than spiral. Its color profile suggests a population of older stars, primarily emitting in the redder wavelengths, although some blue is visible. The galaxy's central bulge is prominent and concentrated, indicative of a high stellar density. There are hints of faint, diffuse features extending outwards, possibly indicative of tidal interactions or past merger events. There is potential ongoing star formation at a low rate, mainly at the edges of the galaxy, based on the bluer color.
