The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile, suggesting a relatively old stellar population. The core region exhibits a yellowish hue, possibly indicative of older stars and reduced star formation activity. Fainter, bluer light extends from the central region, with a slight elongation visible along one axis, potentially revealing a weak disk structure or tidal features. The overall structure appears largely undisturbed, with no major signs of ongoing merger activity. Based on the smoothness of the light distribution, this galaxy is likely an early-type galaxy.
