The galaxy presents as a primarily smooth, elliptical-like object, exhibiting a centrally concentrated light profile. There is a dominant, bright core that fades gradually outward, suggesting a relatively old stellar population. The galaxy's color appears to be moderately red, indicating a lack of significant recent star formation. No spiral arm structures, dust lanes, or other features indicative of ongoing disk activity are visible. The overall morphology appears undisturbed, without major signs of mergers or tidal interactions. The galaxy exhibits a high degree of circularity, with an apparent lack of elongation or asymmetry. The light is uniformly distributed throughout the galaxy's body, except for the prominent core.
