The galaxy presents as a somewhat elliptical, yellowish structure, with a concentrated central bulge indicative of a significant stellar population. The overall color suggests a dominance of older stars, implying a relatively low rate of ongoing star formation. There is a slight asymmetry in the galaxy's profile, potentially resulting from a past interaction or disturbance. The outer regions of the galaxy appear diffuse, fading gradually into the background. A faint, elongated tidal tail seems to extend from the main galactic body, potentially indicating a merging event.
