The galaxy presents as a generally smooth, elliptical form, with a notable central bulge. The core exhibits a high surface brightness, appearing nearly circular with a concentrated luminosity profile that diffuses outwards. There is a hint of a flattened disk-like structure that extends away from the central bulge, though it is not sharply defined and may suggest a more spheroidal shape.

The color gradient transitions from a yellow-white hue in the core to a redder tone in the outer regions. This may imply an older stellar population in the outer parts relative to the core. There are minor disturbances visible that suggests the possibility of a past or ongoing minor interaction/merger. Overall, the galaxy shows signs consistent with a relatively evolved state.
