The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a high degree of central concentration, with a relatively uniform intensity gradient extending outwards. There is a lack of distinct spiral arm structures or other features typically associated with disk galaxies. The galaxy appears to be relatively isolated with no immediately apparent signs of ongoing major mergers, though some minor asymmetry or tidal disturbances cannot be completely ruled out. The color profile is relatively homogenous, with a suggestion of slightly redder hues towards the central regions, potentially indicating an older stellar population. Overall, the galaxy appears to be a relatively massive, evolved system, likely undergoing passive evolution.
