The galaxy presents as a largely smooth, elliptical-like structure with a cigar-shaped morphology. It exhibits a pronounced central bulge that appears yellowish-white in color, indicating a population of older stars. The outer regions of the galaxy are less luminous, displaying a slightly bluer hue, potentially suggesting the presence of some younger stars or regions of low-level star formation, although the overall star formation rate appears to be suppressed. There is no clear evidence of spiral arms or significant dust lanes. Minor disturbances are not present in the structure. The galaxy is relatively compact in size.
