The galaxy presents as a single, dominant object with a relatively smooth and centrally concentrated light profile. It appears to be generally elliptical, with a notable lack of spiral arm structure. The central region exhibits a yellow-white hue, suggesting an older stellar population with minimal ongoing star formation. The outer regions fade into a fainter, more diffuse blue-white halo, possibly indicating the presence of a population of older stars as well as some ongoing star formation at a low rate. There is no obvious evidence of tidal tails, ongoing mergers, or significant dust lanes.
