The galaxy presents as a generally smooth, elliptical form, with a concentrated central bulge. The galaxy's color profile suggests a dominant population of older stars, exhibiting a reddish-orange hue. There are subtle color gradients observed, indicating possible variations in stellar population age across the galactic structure. The overall structure of the galaxy appears relatively undisturbed, with no obvious signs of significant tidal interactions or ongoing major mergers. There may be a minor asymmetry on the lower edge of the disk, implying there could be a minor disturbance occurring. The galaxy is moderately luminous and has a non-negligible rate of star formation.
