The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with no discernible spiral arm structures or prominent dust lanes. The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. The central region exhibits a yellowish hue, suggestive of an older stellar population. The outer regions appear slightly bluer, potentially indicating the presence of a younger stellar population. There is no apparent evidence of ongoing major merger activity or significant tidal disturbances. Based on its morphology, this galaxy is most likely an elliptical galaxy.
