The galaxy presents an elongated, somewhat irregular morphology. The central region exhibits a bright, concentrated bulge, possibly indicative of an older stellar population. Extending outwards from this central bulge, there is evidence of a flattened, disk-like structure, though it appears rather disturbed or diffuse. There are suggestions of faint, blueish spiral arms extending from the bulge. The relative blueness implies ongoing or recent star formation. It is not clear if the slight irregularity of the disk is due to a past or ongoing merger. Overall, the galaxy appears to be a transition object between a elliptical and spiral galaxy.
