The galaxy presents as a single, relatively smooth and concentrated light source. The overall morphology appears elliptical, with a high degree of central concentration. It exhibits a roughly round shape, lacking any obvious spiral arms or prominent disk-like features.

The color profile suggests a dominant population of older stars, indicated by the yellowish-red hue, with a possible smaller fraction of younger, bluer stars in the very central core, indicated by a slightly more green-yellow hue. There is no strong evidence of active star formation on a galaxy-wide scale. The general homogeneity of the light distribution indicates the absence of major ongoing mergers or significant tidal disturbances. There is no evidence of spiral structure or dust lanes.
