The galaxy presents as a fairly smooth, centrally concentrated object, likely an elliptical or lenticular type. Its overall shape appears somewhat elongated, though closer to round than cigar-shaped. There is no strong evidence of spiral arms or significant disk structure visible in the image. The central region exhibits a bright, concentrated glow that gradually fades towards the outer edges. There are no obvious signs of major mergers or tidal disturbances, though the possibility of a minor interaction cannot be ruled out given the resolution. The galaxy exhibits a color gradient, appearing yellower and redder at the core, with the outer regions appearing somewhat more blue. This color difference likely signifies older stellar populations concentrated in the central bulge, with relatively little current star formation. The image quality does limit the detection of any fine details.
