This galaxy presents as a relatively smooth, centrally concentrated object. The core region exhibits a pronounced redder hue, possibly indicative of an older stellar population. Surrounding the core is a more diffuse, bluer envelope. This suggests the presence of a younger, star-forming population in the outer regions. The galaxy appears to be generally elliptical in shape, though it may possess some slight distortions suggesting possible minor interactions or disturbances. There is little evidence of strong spiral arm structure or a prominent dust lane.
