The galaxy presents as a lenticular-like system exhibiting characteristics of both elliptical and spiral morphologies. It displays a primarily smooth, featureless profile, lacking prominent spiral arms or a well-defined disk. The central bulge appears bright and concentrated, with a roughly spheroidal shape. Faint, diffuse extensions are observed surrounding the core. The color profile suggests an older stellar population, with a reddish hue dominating the core and extending outwards. There are areas of bluer light in the surrounding areas, implying the presence of some younger stars. The galaxy exhibits a moderate ellipticity and lacks any signs of major tidal disturbances or ongoing mergers, although a minor disturbance cannot be excluded.
