The galaxy presents a concentrated, yellowish-orange central region that dominates its overall appearance. This core suggests an older stellar population, consistent with a significant amount of evolved stars. The galaxy does not appear to possess well-defined spiral arms; it lacks a structured disk and presents a more amorphous structure. There is a slight irregularity in the shape, possibly indicating a recent or ongoing interaction or merger. A faint extension, or tidal feature, hints at a past gravitational disturbance, although it is not sharply defined. The colour gradient suggests some star formation is happening; however, the central bulge does not appear to be actively forming many new stars. The overall smoothness of the light distribution indicates that this is likely an early-type galaxy.
