The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a slightly elongated, elliptical shape, trending towards a more circular morphology, with only a minor cigar shaped aspect. The light distribution suggests a bulge-dominated system, with a high degree of central light concentration. The color gradient indicates a radial change in stellar populations, with the central region exhibiting bluer colors and a yellow lower portion. There's a notable asymmetry in the light distribution and morphology, potentially indicative of a minor interaction or disturbance affecting the structure. There is also evidence of tidal tails. While the galaxy appears mostly undisturbed, there is a subtle suggestion of ongoing gravitational interactions or recent mergers.
