The galaxy presents as a largely featureless, elliptical-like structure. The light profile suggests a high degree of central concentration, with intensity decreasing gradually outward from a bright core. There is a slight elongation in the shape, deviating from a perfect circle. The color appears generally uniform, with a yellowish hue that may indicate an older stellar population and a relative lack of ongoing star formation. There is a subtle color gradient from the inner region to the outer edges. The galaxy lacks any discernable spiral arms, dust lanes, or other prominent features typically associated with disk galaxies. It appears undisturbed, showing no signs of recent or ongoing mergers or tidal interactions.
