The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, indicative of a substantial stellar population and potentially an active galactic nucleus. There is a noticeable color gradient from the center outwards, shifting from a yellowish-white towards a bluer hue in the outer regions. This suggests the presence of younger, hotter stars in the surrounding disk, though it is not distinctly disc-shaped. The overall shape is somewhat elongated. There is no apparent evidence of major mergers or tidal disturbances affecting the galaxy's morphology. The galaxy appears to be relatively isolated in its environment, without any clear signs of interactions with nearby galaxies in the immediate vicinity. The galaxy displays a moderate redshift, indicating a significant cosmological distance. Star formation within the galaxy is estimated to be relatively subdued, with a low specific star formation rate.
