The galaxy presents a generally smooth morphology, with a centrally concentrated luminosity profile. It appears elliptical in shape, exhibiting an elongated structure. The core region shows a yellowish hue, possibly indicating an older stellar population. Fainter, bluer extensions are observed at the periphery, potentially signifying younger stars or ongoing star formation, though at a low rate. No distinct spiral arms or significant dust lanes are discernible. There are hints of minor disturbances in the outer regions, though it does not appear to be undergoing a major merger.
