The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. The color profile indicates a higher concentration of older stellar populations, suggesting relatively low recent star formation. There is an apparent secondary structure, slightly less luminous and similarly colored, in close proximity to the primary galaxy. This could potentially be a smaller satellite galaxy or tidal debris indicative of a minor interaction or past merger event. The overall morphology suggests a relaxed system, although the potential interaction warrants further investigation.
