The galaxy presents a primarily cigar-shaped morphology. A distinct central bulge exhibits a concentrated yellowish-orange hue, suggesting an older stellar population. This contrasts with the fainter, bluer light emanating from the more extended regions of the galaxy, possibly indicative of ongoing star formation. These regions seem to be parts of a disk structure. Evidence of minor disturbances is visible as distortions, possibly indicating minor gravitational interactions. The galaxy appears relatively smooth in the central bulge. 
