The galaxy presents as a relatively smooth, elliptical form. It exhibits a central bulge that is bright and concentrated, with a slightly elongated shape. The color distribution suggests a population of older stars, with a yellowish-red hue dominating the central region. The outer regions of the galaxy gradually fade, showing a bluer tint, possibly indicative of some younger star formation. No distinct spiral arms or prominent dust lanes are discernible in this image. The galaxy does not appear to be strongly interacting with any other nearby galaxies. There is no evidence of major tidal distortions or prominent starburst activity.
