The galaxy presents as a moderately luminous object with a central bulge. Its morphology appears to be intermediate between elliptical and spiral, possibly a lenticular galaxy. The central region exhibits a yellowish hue, potentially indicating an older stellar population. Fainter, bluish light extends outwards, which could be indicative of more recent, though not prolific, star formation activity in the outer regions. The disk or extended structure of the galaxy is somewhat diffuse. There is no definitive evidence of a major ongoing merger, but some minor disturbances may be present in the outer regions. Overall, it appears to be a relatively quiescent galaxy, with a substantial mass, and subdued star formation.
