The galaxy appears as a relatively smooth object, exhibiting a somewhat rounded morphology. A central bulge is suggested, displaying a yellow-orange hue, potentially indicating an older stellar population. The outer regions exhibit a bluer tint, suggestive of younger stars. The presence of subtle irregularities hints at possible tidal interactions or ongoing mergers. Some light is more concentrated than others. Overall, this galaxy presents a complex combination of features, likely representing a system undergoing significant evolutionary processes.
