The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with a notable concentration of light toward its center. There is some indication of possible tidal features, with some asymmetry that may be caused by the early stages of a minor merger. The galaxy's color profile suggests a population of older stars, given the redder hue in the core, although some regions appear bluer, possibly indicating more recent or ongoing star formation. It has a generally rounded shape, though not perfectly circular, with an apparent deviation from a spherical form.
