The galaxy exhibits a generally elliptical morphology, appearing relatively compact with a concentrated central region. The light distribution indicates a fairly smooth overall structure, although there seems to be some irregularity or faint extension visible in the immediate vicinity, possibly suggesting a minor disturbance of its structure. The color gradient suggests the presence of a more evolved stellar population dominating the outer regions as we see more red color there, while the central region contains bluer, younger stars. The overall color profile indicates ongoing or recent star formation, but the smooth appearance points to a possible early-type or lenticular galaxy classification. The irregularities could also be signs of gravitational interactions or accretion events.
