The galaxy presents as a relatively smooth object, appearing somewhat elliptical in shape though near round. It exhibits a concentrated central bulge that diminishes in luminosity moving outwards. The galaxy's color profile indicates a yellow-white hue in the core region, transitioning to a bluish-white disc component. There is a suggestion of ongoing interaction or possibly a merger, which could be considered a second nucleus in the lower portion of the galaxy which is exhibiting bluer colors suggestive of ongoing star formation. There are no obvious signs of strong tidal tails or distorted morphology that would indicate a recent major merger.
