This galaxy exhibits a roughly elliptical morphology, although some features suggest ongoing interaction or internal disturbances. The central region displays a concentrated, yellowish-orange luminosity profile, potentially indicative of an older stellar population dominating the core. There is evidence of bluer regions, especially one to the left of the nucleus, possibly representing areas of more recent star formation. The overall distribution of light implies a system that is not perfectly smooth; there appear to be irregular features or substructures within the galactic disk. The galaxy shows a degree of asymmetry, which may indicate a minor merging event or tidal disturbance in its recent history.
