The galaxy appears as a fairly round, centrally concentrated object with a smooth light distribution. There is a slight color gradient, trending from a whiter core to a bluer, more diffuse outer region. The galaxy lacks any obvious spiral arm structure or distinct morphological features. The observed characteristics suggest that it is likely an elliptical galaxy, possibly with ongoing, but relatively low, star formation in its outer regions. There is no apparent evidence of any major interactions or mergers.
