The galaxy presents as a moderately luminous object with a discernible disk-like morphology. It appears moderately smooth, with some indication of internal structure. The main body is generally elliptical and appears to be in a later stage of formation. While there is no strong central bulge, the inner region does appear to be more densely populated with stars. Faint spiral arm structures are potentially visible, but it is difficult to tell due to the angle of the object. There is some indication of star formation within, as the galaxy seems to be more blue-shifted compared to red. There is a potential merging event or tidal disturbance occurring on the right side of the galaxy.
