The galaxy appears to be a relatively compact elliptical galaxy, exhibiting a smooth, featureless morphology with a high degree of central concentration. The light profile appears to follow a Sersic profile, with an index implying a steep decline in surface brightness away from the center. It exhibits a subtle elongation, with a slight deviation from perfect circularity. The galaxy displays a color gradient, with the core appearing more yellow than the outer regions, suggesting a population of older stars dominating the central regions. Overall, the galaxy's appearance indicates a passively evolving system with little to no ongoing star formation.
