The galaxy presents a generally smooth morphology, appearing largely elliptical in shape, with a bright central bulge. There is a subtle disc component present. The galaxy exhibits a concentration of light towards the center, suggesting a relatively old stellar population, particularly in the bulge. The overall color profile implies a range of stellar ages. There are no strong indications of active star formation, major mergers, or significant tidal disturbances. However, there may be some minor disturbances visible. The overall structure does not deviate significantly from that of a typical early-type spiral or lenticular galaxy.
