The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish hue, suggesting a population of older stars. A slight elongation is observable along one axis, deviating minimally from a perfectly circular shape. There is no visible evidence of spiral arms, dust lanes, or significant star formation regions. Fainter, diffuse extensions are noted surrounding the central region, implying a gradual decline in stellar density towards the outer limits of the galaxy. No signs of tidal tails or recent merger activity are apparent within the field of view, further supporting a relatively undisturbed evolutionary history.
