The galaxy presents a predominantly elliptical morphology, though it does display some features suggestive of a disk component. The central region exhibits a bright, concentrated bulge with a yellowish hue, indicating a population of older stars. Moving outwards, the color shifts towards a slightly bluer tint, hinting at the presence of younger stellar populations and ongoing, though potentially moderate, star formation activity. The overall shape appears moderately rounded. There is a minor asymmetry detectable in the outer regions, potentially indicating a past or ongoing interaction. No strong tidal tails or signs of a major merger are readily apparent. The galaxy appears relatively undisturbed, although subtle irregularities suggest minor gravitational disturbances might be present.
