The galaxy presents a primarily smooth morphology, though it exhibits features suggesting potential disturbance or interaction. The central region appears bright and concentrated, likely indicating a significant stellar population or active galactic nucleus. There is evidence of a fainter, elongated structure extending from the central region, which could represent a tidal tail or a distorted galactic arm. The color gradient within the galaxy suggests variations in stellar populations or dust content, with bluer hues concentrated in the center and redder tones dominating the extended structure. The overall asymmetry of the galaxy hints at a possible ongoing or recent merger event, or perhaps interaction with a smaller companion galaxy. Overall, this galaxy seems to be an elliptical galaxy experiencing a possible merging event, or significant disturbance.
