The galaxy presents as a relatively smooth, elliptical-like structure, with a highly concentrated central bulge. The light distribution appears circularly symmetric. There is a distinct colour gradient visible, with the central region exhibiting a yellow-orange hue, potentially indicative of an older stellar population. This contrasts with a fainter, more diffuse outer region exhibiting a bluer tint, suggestive of some star formation processes, albeit at a low rate. No significant spiral arm structures or strong tidal disturbances are apparent. The galaxy appears largely isolated, with no obvious signs of major ongoing or recent merger activity. Overall, the galaxy seems to be a well-formed, evolved system.
