The galaxy appears as a relatively smooth and centrally concentrated object. Its overall form is elliptical, lacking any prominent spiral arm structures. The light distribution appears quite uniform throughout the galaxy, without any distinct bright knots or areas of intense star formation readily visible. This suggests a stellar population dominated by older stars and a relatively low current star formation rate. There is a slight elongation to its shape, but it's mostly round. There are no signs of any major mergers or tidal disturbances, indicating that it is likely a relatively undisturbed system.
