The galaxy presents a roughly elliptical morphology, viewed approximately edge-on. A bright, concentrated central bulge is evident, exhibiting a smooth luminosity profile, suggesting an older stellar population in this region. Fainter disk-like extensions protrude from either side of the bulge.

The disk displays a slight asymmetry in the distribution of light. There is a hint of non-uniformity that possibly indicates the presence of spiral arm structure or dust lanes, however, it is difficult to resolve this in the image. Some localized areas of more intense emission are observed in the disk, which may correspond to regions of active star formation. A small, very faint tidal tail or bridge may be present to the left of the galaxy. 
