The galaxy appears to be an elliptical or lenticular type, characterized by a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The galaxy's overall shape is elongated, displaying a moderate ellipticity. A faint, diffuse halo surrounds the central region, extending outwards and gradually fading into the background. There is a slight hint of a disk-like structure, but it is not clearly defined. Evidence suggests a possible minor disturbance of the galaxy structure. The galaxy shows a very low rate of new star formation.
