The galaxy presents a generally elliptical morphology, appearing largely smooth with a high degree of central concentration. The light profile suggests a well-defined spheroidal component, with a minor contribution from a possible disk. The galaxy's color exhibits a gradient, with the core region appearing more yellow-red, indicating a population of older stars. Fainter blue emission regions are present suggesting areas of recent star formation, these are confined to a small region of the galaxy. There is evidence of a potential tidal feature, possibly a tail or bridge, suggesting a past interaction or merger event, this lies to the top of the galaxy. Overall, the galaxy appears to be in a transition phase, possibly moving from a star-forming spiral to a passive elliptical.
