The galaxy presents as a somewhat flattened disk, viewed nearly edge-on. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting an older stellar population likely dominated by red giant stars. Moving outward from the bulge, the disk appears bluer, indicating the presence of younger, hotter stars and ongoing star formation. The disk structure appears relatively smooth with hints of faint spiral arm structure. There appears to be a small disruption on one side of the galaxy that could be an area of new star formation. The overall morphology suggests this galaxy is either a lenticular or spiral galaxy, with a moderate amount of star formation.
