The galaxy presents a generally smooth, elliptical morphology. It exhibits a pronounced elongation, appearing cigar-shaped. The color distribution is not uniform, with a central concentration of yellowish-white light, suggesting an older stellar population. Fainter, bluer light is observed in the outer regions, potentially indicative of some ongoing, albeit limited, star formation. There is some evidence of a minor disturbance or interaction; though not a full merger, the morphology is not perfectly regular. Overall, this galaxy appears to be a moderate-mass system, potentially undergoing a slow transition in its star formation history.
