This galaxy exhibits a morphology that suggests a relatively smooth structure, though some features are present. The shape appears to be in between round and elliptical, showing some degree of elongation, but not a highly defined disk structure. It has a reddish hue, indicating a stellar population that is primarily composed of older stars, with reduced ongoing star formation. There appears to be a nearby object that could indicate an ongoing or past interaction. The tidal features may be disrupting the morphology of the galaxy. There may be a secondary object close enough to be in the merging process.
