The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and featureless appearance. The light distribution suggests a centrally concentrated luminosity profile, with the brightest region located at the core. There is a gradual decrease in surface brightness moving outward from the center, without any prominent spiral arms or distinct dust lanes visible in this image. The shape is elongated, but not extremely so, exhibiting an intermediate ellipticity. There is no clear evidence of any ongoing major merger activity, such as tidal tails or strong distortions in the overall structure, but there is minor disturbance of sorts in the overall form. There appears to be a slight color gradient with a yellowish core that transitions into a reddish halo, consistent with an aging stellar population, with a weak rate of star formation.
