The galaxy presents a largely smooth and rounded morphology, suggestive of an elliptical or lenticular type. It displays a central concentration of light, exhibiting a bright core that diminishes outwards. The overall color profile leans towards the redder end of the spectrum. There's no immediately discernible evidence of spiral arms, prominent dust lanes, or ongoing major mergers. The smooth appearance indicates a population of older stars and potentially reduced recent star formation activity. There may be minor tidal disturbances, but the galaxy appears largely undisturbed.
