The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests minimal spiral arm structure or prominent dust lanes. The color profile indicates an older stellar population, with a yellowish-red hue dominating the bulge and inner regions. The outer regions exhibit a slightly bluer tint, possibly indicating more recent star formation, but this is subtle. The overall morphology suggests a relaxed system without significant tidal disturbances or ongoing major mergers. It is somewhat round in appearance, though potentially slightly elongated.
