The galaxy presents a generally smooth, elongated morphology. The central region exhibits a concentration of light, appearing yellowish-orange, suggestive of an older stellar population. Fainter, bluer light emanates from the outer regions, hinting at some ongoing star formation. The galaxy shows no distinct spiral arms or bar structure and there is no evidence of a major merger occurring. There is only slight evidence of minor tidal disturbances or interactions. The overall shape appears to be somewhat cigar-shaped.
