The galaxy presents a generally smooth and elliptical morphology. The light distribution suggests a centrally concentrated spheroid. The color profile is suggestive of an older stellar population, with a yellowish hue dominating the central region, becoming slightly redder toward the outer edges. There is no apparent disk structure or spiral arm features visible. I do not see evidence of strong tidal interactions or ongoing mergers, but a minor asymmetry in the outer regions could suggest a previous interaction or disturbance. The object exhibits a high degree of circularity with its shape appearing nearly perfectly round.
