The galaxy presents a largely smooth morphology. Its shape appears generally elliptical, though not perfectly round, tending towards an intermediate spheroidal form. There is little evidence of prominent spiral arms or a well-defined disk structure. The light distribution indicates a centrally concentrated bulge, with a gradual fall-off in luminosity towards the outer regions. The galaxy's color is broadly consistent with a population of older stars, with some indication of ongoing, but low levels of star formation. There may be minor tidal disturbances, though these are not overwhelmingly pronounced. Overall, the galaxy appears relatively undisturbed, displaying a structure that has evolved without major recent interactions or mergers.
