The galaxy presents as a somewhat smooth, elongated spheroid. Its core exhibits a bright, concentrated central bulge with a reddish-white hue, suggesting a population of older stars. Extending outwards from the core, a diffuse, fainter halo is visible. This halo exhibits a bluer tint than the core, perhaps indicating a population of younger stars or ongoing star formation in the outer regions. There's little evidence of spiral arm structures or prominent dust lanes. The overall color distribution indicates a galaxy that is potentially transitioning, exhibiting characteristics of both early-type and late-type galaxies. There is no indication of a recent major merger event. Subtle irregularities in the outer regions may suggest minor gravitational disturbances or past minor interactions. The galaxy appears to be relatively isolated within its environment.
