The galaxy presents as a somewhat amorphous, centrally concentrated object with a smooth appearance. Its light distribution suggests a spheroid morphology, with no obvious spiral arm structure or prominent disk features discernible within the resolution limits. The core region appears to be brighter and possibly more densely populated. There is a hint of tidal or merger activity, with some degree of distortion. The color index suggests a mature stellar population. Overall, the galaxy has a round shape.
