This galaxy appears as a relatively smooth, elliptical-like structure. It has a concentrated central bulge that is noticeably brighter and more yellow in color, suggesting a population of older stars. The outer regions of the galaxy exhibit a more diffuse and slightly bluer hue, indicating the presence of younger stars and possibly some ongoing star formation, although it appears to be at a low rate. The galaxy lacks any obvious spiral arm structures or significant dust lanes. Its overall shape seems mostly round with a slight elongation. There is no evidence of major ongoing mergers or significant tidal disturbances, although there may be some minor irregularities in the outer regions. The galaxy is a fairly massive system, and its stellar population is dominated by older stars, with a lower amount of star formation ongoing.
