The galaxy presents as an elliptical morphology, displaying a smooth and centrally concentrated light profile. It exhibits a generally homogenous color distribution, trending towards yellowish-white. There appears to be a slight elongation, deviating from a perfectly circular form. The galaxy does not display any obvious spiral arm structures, star-forming regions, or significant dust lanes. The overall appearance suggests a relatively evolved system with a dominant population of older stars. There is no visual evidence to indicate recent or ongoing major merger activity, though minor disturbances cannot be ruled out. The galaxy is of intermediate size, with a moderate apparent brightness.
