The galaxy appears to be an elliptical type, presenting a smooth, centrally concentrated luminosity profile. It exhibits a yellowish-white hue in its core, suggesting an older stellar population dominated by redder stars. The overall shape tends towards round, though it appears slightly elongated, with a minor axis shorter than its major axis. There is little evidence of spiral arm structure or dust lanes. No signs of any ongoing major mergers, though there is a very slight possible asymmetry in the outer regions, which could indicate past minor interactions or disturbances. Overall, it appears as a relatively evolved system with high mass and ongoing star formation, although at a reduced rate compared to actively star-forming galaxies.
