The galaxy presents a generally smooth appearance with a concentrated central bulge and a faint, disk-like structure. The light distribution suggests a predominantly older stellar population, evidenced by the reddish-yellow hue of the central bulge. The disk exhibits a bluer tint, hinting at the presence of some younger stars.

There is a slight asymmetry in the galaxy's morphology, with a subtle extension or plume emanating from one side. This feature could potentially be indicative of a past minor interaction or a tidal disturbance. Given the overall smoothness, the disturbance appears relatively minor or ancient. No strong indications of active star formation are readily apparent from this image, but the slight bluer color in the surrounding disk means there is most likely *some* star formation. The galaxy's shape is predominantly round, with minimal elongation observed. There is no evidence of a recent or ongoing major merger.
