The galaxy presents as an elliptical morphology, appearing somewhat elongated with a smooth, diffused light distribution. A bright central bulge dominates the luminosity profile, suggesting a high concentration of older stellar populations. Fainter, extended halos are also present. Subtle color gradients are observed, with the central region appearing slightly yellower, possibly indicating older stars and a lower rate of star formation. The general structure shows no distinct spiral arms or prominent dust lanes. There is no significant presence of any ongoing merging events. The galaxy's shape suggests a lack of significant rotational support.
