The galaxy presents an elongated, somewhat cigar-shaped morphology. A significant portion of the galaxy's luminosity is concentrated in a central, brighter region that could be described as smooth. This suggests the presence of a galactic bulge, possibly containing an older stellar population. Fainter, diffuse light extends from this central region, tracing the outer structure of the galaxy. The smoothness fraction indicates a predominantly smooth appearance, however there is a region of minor disturbance present. It is difficult to discern a distinct disk structure. Overall, the galaxy exhibits characteristics that place it somewhere between a smooth elliptical and a disk galaxy.