The galaxy presents as a moderately bright, elongated structure with a relatively defined core region. There is evidence of a disk component that is observed at an oblique angle relative to the observer's line of sight.

The central region exhibits a bright core and a darker ring that is more pronounced. This suggests potential obscuration from dust within the galaxy's disk. Color variations are apparent across the galaxy, with a noticeable color gradient from the central region outwards, where there appears to be a faint, blue color gradient at the upper and lower edge of the ring.

Based on the morphology, the object does not appear to have undergone a major merger event recently. The overall morphology is not particularly smooth, implying the presence of some internal structure within the galaxy. The shape appears roughly elliptical overall, with an estimated diameter of about 20 arcseconds.
