This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated light profile, with the luminosity decreasing gradually toward the outer regions. The core region appears yellowish, suggesting an older stellar population. No distinct spiral arms or prominent dust lanes are visible. There is a very slight hint of bluer light on one side of the galaxy, suggesting the possibility of minor, ongoing star formation, but it's predominantly composed of older stars. Its overall morphology is smooth and round. There is no evidence of any major disturbances or ongoing mergers.
