The galaxy presents as a fairly smooth, elliptical object, exhibiting a concentrated central bulge that transitions outwards into a more diffuse halo. The core region has a yellowish hue, suggesting an older stellar population. Surrounding this central area, there is a subtle presence of bluer light, possibly indicating some ongoing star formation. The galaxy appears to be relatively isolated, without obvious signs of major tidal interactions or significant morphological disturbances, suggesting the presence of a gravitationally settled and largely undisturbed system.
