This galaxy appears to be a relatively smooth and centrally concentrated system. The light is somewhat elliptical in shape, presenting as a flattened spheroid, more like a cigar than a circle. A central bulge appears bright and dominant, transitioning outwards into a fainter, diffuse halo of light. Hints of disk-like features are subtle but visible, with possible spiral arm structures loosely wound around the central bulge.

The color distribution shows a gradient from a bluer disk area towards a redder bulge. This suggests that the bulge likely contains an older stellar population compared to the disk which shows that younger stars are present. The galaxy appears to be relatively undisturbed, with no major signs of tidal interactions or ongoing mergers. There are small, possible areas of minor disturbance present.
