The galaxy presents as a roughly elliptical structure, exhibiting a smooth and concentrated central bulge. There is a general lack of distinct spiral arm features. The galaxy appears largely spheroidal with moderate ellipticity. Color analysis suggests a relatively evolved stellar population. The central region is characterized by a yellowish hue, likely indicating older stars. There is an absence of significant dust lanes or prominent star-forming regions based on the lack of patchy coloration. The galaxy appears to be relatively isolated with no immediately obvious signs of major tidal interactions or recent mergers, however, there may be very minor disturbances present within the structure. The overall appearance is consistent with an early-type galaxy, likely an elliptical or lenticular galaxy at a considerable distance.
