The galaxy presents as a single, relatively smooth object with a concentrated central bulge. There is minimal discernible structure such as spiral arms or a prominent disk. The object appears to be largely spheroidal, approaching elliptical morphology, with only a slight deviation towards an elongated shape. Its color profile indicates a higher concentration of older stars, shifting toward the redder portion of the spectrum. However, there is also a bluer halo, suggesting some ongoing, albeit limited, star formation. There is no evidence of significant tidal distortions or ongoing major mergers. Subtle irregularities could indicate a minor interaction or internal disturbances within the galaxy, but these are not pronounced. The overall impression is of a fairly settled, massive galaxy.
