The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated luminosity profile. The core region is bright and diffuse, transitioning gradually to a fainter, less structured halo. There's minimal evidence of spiral arm structures. The overall color is suggestive of an older stellar population, lacking the distinct blue hues associated with significant ongoing star formation. Subtle color variations within the galaxy might indicate variations in stellar density or composition, but these are not pronounced. There is a possible minor disturbance or asymmetry present in the morphology.
