The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades into an extended halo. The color gradient transitions from a bright, yellowish core to a slightly redder outer region. No distinct spiral arms or prominent dust lanes are apparent. There is a slight elongation, but overall, the object appears relatively round, with no evidence of major ongoing mergers or significant tidal disturbances. Faint, diffuse features may be present, indicative of minor interaction or past merger events, though difficult to determine from the provided image resolution. The overall structure suggests a relatively evolved system with diminished star formation activity.
