The galaxy presents an elliptical morphology, displaying a smooth, centrally concentrated light profile. The core region exhibits a yellowish hue, indicative of an older stellar population. Moving outward from the core, the color transitions to a bluer shade, suggesting the presence of younger stars. There appears to be a subtle disk-like structure present, with a slight elongation. There are no obvious signs of a major ongoing merger event, though there may be a minor disturbance in the outer regions. The galaxy exhibits moderate luminosity.
