The galaxy presents a predominantly smooth morphology, with a notable central bulge region exhibiting a concentrated luminosity profile. The overall form appears elliptical, tending towards an intermediate ellipticity rather than a perfectly circular or highly elongated shape. There are suggestions of faint, diffuse features extending from the central region, possibly indicative of a faint disk or tidal interactions, but no clear spiral arm structures or prominent dust lanes are discernible. The color profile is relatively uniform, with a slight redder hue concentrated within the core, suggestive of a population of older stars. No indications of a major ongoing merger event or strong tidal disturbances are apparent, though minor interactions cannot be entirely ruled out based on the faint outer structures. Overall, the galaxy appears to be a fairly massive, relatively quiescent system, possibly undergoing low levels of star formation.
