The galaxy presents as a flattened, elliptical structure with a distinct bulge. The central region exhibits a concentrated luminosity, appearing yellowish-white, suggestive of an older stellar population. Moving outward, the disk displays a bluer hue, indicative of more recent star formation. The galaxy shows signs of being slightly elongated, with the major axis significantly longer than the minor axis. There is a subtle asymmetry in the outer regions, potentially indicating a gravitational interaction or minor disturbance, but it mostly appears as a smooth structure.
