The galaxy exhibits a generally smooth morphology with a slight bluish tint along its primary axis, suggestive of ongoing, but potentially weak, star formation. The overall shape appears to be somewhere between round and elliptical, with a slight elongation. There is evidence of a possible minor interaction or disturbance; the galaxy appears to have a somewhat asymmetrical structure. There is a noticeable redder region at one end of the galaxy, which could indicate an older stellar population in that area.
