The galaxy appears as a somewhat diffuse, centrally concentrated object. Its overall morphology suggests a relatively smooth structure, with a possible slight elongation. The color distribution reveals a central region exhibiting a yellowish to whitish hue, possibly indicative of an older stellar population. There is evidence of fainter, reddish components in the surrounding regions, which might suggest the presence of some areas with active star formation or older, redder stars. The overall structure suggests this galaxy could be an elliptical or lenticular galaxy. There seems to be no evidence of active merging, but there could be minor disturbances in the galactic structure.
