The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a centrally concentrated light profile, appearing brightest at the core and gradually diminishing outwards. The overall shape is elongated, deviating somewhat from a perfect circular form, but is closer to round than it is to cigar shaped. There is no discernible spiral arm structure or significant dust lane features visible within the galaxy's disk. The galaxy appears mostly undisturbed with no signs of major mergers. The general color profile suggests a moderate population of older stars, consistent with an intermediate stage of stellar evolution.
