The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Its overall shape leans towards being classified as somewhere between round and slightly elongated. There is minimal evidence of a prominent disk structure or spiral arms. Subtle variations in color suggest varying stellar populations, possibly with younger, bluer stars sparsely distributed throughout the galaxy, in contrast to the more yellow and red hues concentrated in the center. There's no immediately apparent evidence of major merging activity or significant tidal disturbances, although there are indications of some minor disturbances. The galaxy's light appears to be quite diffuse, suggesting that it has a relatively extended halo. It appears to be a generally quiescent system, with a relatively modest star formation rate.
