The galaxy presents as an elliptical morphology, exhibiting a smooth and concentrated distribution of light. The central region appears bright and yellow-orange in color, suggesting a population of older stars. Fainter, diffuse greenish light surrounds the core, possibly indicative of some ongoing, though limited, star formation activity. The galaxy exhibits a generally round shape, with only very slight elongation. There is no clear evidence of spiral arms or significant dust lanes, nor signs of any major interaction or ongoing merger event, although a minor disturbance cannot be completely ruled out. The overall structure suggests a relatively evolved system.