The galaxy presents as an elliptical or lenticular galaxy with a smooth, centrally concentrated light profile. Its shape is generally round, with only a slight deviation from perfect circularity. The central region exhibits a bright, concentrated core, likely indicative of an older stellar population.

A faint, diffuse halo surrounds the central region, its color and shape consistent with the galaxy being either elliptical or lenticular. There is no clearly discernible disk component nor spiral arm structure visible in this image. There is no distinct dust lane apparent, further suggesting it's not a spiral galaxy. There is no major asymmetry or obvious tidal feature indicating any ongoing major interaction or recent merger event, but a slight disturbance is possible.
