The galaxy presents a flattened, elongated morphology, suggesting it is either a spiral viewed edge-on or an elliptical galaxy with some degree of flattening. It exhibits a bright, concentrated central bulge, which appears yellowish, indicative of an older stellar population. Fainter, bluer light emanates from the disk region, suggestive of ongoing star formation, although the presence of prominent spiral arms is not apparent at this resolution. Dust lanes are subtly visible, further supporting the presence of a disk structure. Overall the galaxy appears to have some degree of disturbance, with subtle asymmetries in the outer regions, and a slightly disturbed morphology.
