The galaxy presents as a somewhat face-on spiral or lenticular system. There is a distinct bulge region that is an elliptical, pale yellow and concentrated at the center of the system. This likely indicates an older stellar population within the bulge. The spiral arms, if present, are not clearly defined, but there is a bluer diffuse light extending outwards from the bulge, suggestive of ongoing or recent star formation within the disk. The overall shape appears to be somewhere between round and elongated, and the galaxy doesn't show any obvious signs of major interactions or mergers, though there may be a minor disturbance indicated by slight asymmetries in the outer regions. The galaxy appears relatively smooth in texture, with some hints of disk-like features.
