This galaxy exhibits a predominantly smooth morphology, appearing as an elliptical or lenticular type. Its shape is largely consistent with an intermediate ellipticity, deviating slightly from perfectly round. The galaxy displays a distinct central bulge, which appears brighter and more concentrated than the surrounding disk. The light from the core suggests the presence of an older stellar population. Faint, diffuse outer regions are visible, gradually fading into the background.

There may be some minor tidal disturbances, and possibly a faint disk, as indicated by its slight elongation. There may be ongoing or recent minor merger activity. The color profile suggests a redder, evolved stellar population with limited ongoing star formation.
