The galaxy presents as a moderately bright, elliptical structure with a concentrated central bulge exhibiting a yellowish hue, likely indicative of an older stellar population. The main body of the galaxy is extended, with a noticeable elongation suggesting a flattened spheroidal shape. It exhibits a smooth appearance, with no apparent spiral arm structure or significant dust lanes visible at this resolution. There may be a very subtle hint of disk-like structure. Faint bluish regions are observed within the galaxy's halo, possibly hinting at ongoing, though subdued, star formation. There appear to be no signs of major tidal disturbances or ongoing mergers.
