The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, bright and yellow-orange, suggesting a population of older stars. The outer regions of the galaxy appear more diffuse and redder, possibly indicating a declining stellar population or dust absorption. The galaxy is elongated, displaying a cigar-like shape. There is no clear indication of spiral arm structure or significant tidal disturbances, and it appears to be a relatively isolated system. Its overall color suggests low ongoing star formation activity.
