The galaxy presents a generally smooth appearance, lacking prominent spiral arms or a well-defined disk structure. It appears somewhat elliptical in shape, leaning towards an elongated form rather than perfectly circular. The light distribution is concentrated towards the center, with a gradual decrease in intensity moving outwards, suggesting a bulge. There's a subtle color gradient visible, with the central region appearing slightly yellower or redder than the outer regions, potentially indicating an older stellar population concentrated towards the core. Faint irregularities are present, but they do not suggest any major ongoing merger events. The galaxy appears to be relatively isolated, without obvious signs of tidal interactions or close companions.
