The galaxy appears to be a relatively smooth, elliptical-like structure, though some evidence of a disk may be present. It exhibits a subtle elongation, with the major axis significantly longer than the minor axis, giving it a somewhat cigar-shaped appearance. The color profile suggests a population of older stars, as indicated by the dominant reddish-yellow hue, particularly concentrated towards the center. Fainter greenish-blue tinges are present around the periphery, potentially indicative of more recent, though subdued, star formation activity. No significant tidal features or signs of ongoing major mergers are readily apparent. Minor disturbances cannot be ruled out. The galaxy's overall morphology is relatively undisturbed.
