The galaxy presents as a diffuse, centrally concentrated object. The overall color appears somewhat reddish, potentially indicative of an older stellar population and/or dust extinction. It exhibits a relatively smooth morphology, with a slight elongation but without any clear spiral arm structure or strong bar features. There appears to be a subtle hint of a disk, but it is not well-defined. No signs of recent or ongoing major mergers or significant tidal disturbances are evident in the immediate vicinity of the object.
