The galaxy appears to be a relatively smooth, elliptical or lenticular type galaxy. It presents with a centrally concentrated bulge that fades gradually into a surrounding halo of stars. The galaxy has a slight elongation, appearing more "in-between" than perfectly round or cigar-shaped. There is no apparent spiral arm structure or prominent dust lanes visible. The color profile indicates the presence of older stellar populations, with the core appearing redder in color than its surrounding regions, suggesting a lack of recent star formation. The overall structure appears undisturbed, with no signs of major mergers or significant tidal distortions. There are no apparent nearby companion galaxies that could be influencing its morphology.
