This galaxy presents as a relatively smooth, centrally concentrated object. The morphology is largely elliptical, appearing mostly round with only a slight deviation from perfect circularity. There is no apparent spiral arm structure or a distinct disk. The galaxy exhibits a bright, yellowish core, indicating a high concentration of older stars in the central bulge. The color profile suggests a dominant population of older stars, although there may be ongoing star formation activity at a low level, contributing to the slightly bluer outer regions. The smooth appearance indicates that the galaxy is likely a relatively evolved system, having undergone significant dynamical relaxation. There is no evidence of any major mergers or significant tidal disturbances in the immediate vicinity, although there is a small suggestion of minor interactions.
