The galaxy appears as a compact, elliptical-like structure with a relatively smooth, albeit somewhat disturbed, morphology. It exhibits a redder hue, suggesting a population of older stars and a lower rate of ongoing star formation. The concentration of light toward the center is significant, indicative of a massive galactic core. There is evidence of potential tidal features or minor disturbances, such as faint asymmetries in the light distribution, possibly resulting from past interactions or mergers. The object presents a concentrated, bulge-dominated appearance with limited visible disk-like structures.
