The galaxy presents as a smooth, elongated object, potentially an elliptical galaxy or a highly inclined spiral. The central region exhibits a slightly brighter and more concentrated luminosity, indicating the presence of a galactic nucleus or bulge. There is a subtle color gradient across the galaxy, shifting from a slightly redder hue in the central region to bluer tones towards the outer edges. This could suggest differing stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars in the outer regions. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger activity or significant tidal interactions. Faint extensions or diffuse halos may exist beyond the main body of the galaxy, but their visibility is limited by image resolution and signal-to-noise ratio. The light distribution along the major axis seems to gradually fade out.
