The galaxy presents as a relatively smooth, elliptical-like structure. Its core is distinctly bright and concentrated, emitting a yellowish-white light, suggesting a population of older stars. This central bulge is surrounded by a more diffuse halo. The halo exhibits a color gradient transitioning from a pale yellow-white near the core to a bluer hue in the outer regions. This might indicate the presence of younger star formation occurring further away from the galactic center. The galaxy's overall shape appears elongated, possibly suggesting a cigar-shaped morphology. There are no obvious signs of ongoing major mergers or strong tidal disturbances, though subtle irregularities cannot be ruled out at this resolution. The galaxy appears relatively isolated.
