The galaxy presents a centrally concentrated light profile, suggesting an elliptical morphology or a spiral galaxy seen face-on with a dominant bulge. It appears to be a relatively smooth, round structure with hints of minor disturbances, potentially indicative of a past or ongoing interaction or merger. Some of the irregularities around the central core are likely tidal disturbances due to interaction with another galaxy. The galaxy exhibits a reddish-yellow hue, indicating a population of older stars and a lack of significant ongoing star formation. The surrounding region shows faint companions or merging structures, supporting the hypothesis of an ongoing interaction. The overall structure appears to be relatively compact given its estimated luminosity.
