The galaxy presents as a moderately concentrated, elliptical-like structure. A subtle yellowish hue dominates its central region, possibly indicating an older stellar population, or dust extinction. The outer regions appear slightly less defined and fainter, lacking distinct spiral arm structures or prominent star-forming regions.

There is a slight asymmetry, potentially suggestive of a past or ongoing minor interaction with another galaxy or the result of internal dynamics. However, no obvious tidal tails or strong distortions are visible. The object appears relatively smooth and rounded in overall morphology. There may be a hint of faint disk.
