The galaxy presents as a moderately luminous, elongated structure. Its morphology is predominantly smooth with a central, highly concentrated bulge that exhibits a yellowish-white color gradient, suggesting an older stellar population. Fainter, bluer hues extend along the galactic disc, indicative of more recent star formation events, albeit at a relatively low rate. The overall shape is somewhat cigar-like, lacking a distinct spiral arm structure. There is no immediately apparent indication of a major ongoing merger event, although there is very slight possible disturbance in the overall structure.
