The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. The light is concentrated towards the center, displaying a bright, yellowish core, which is indicative of an older stellar population. There is a slight color gradient, with the inner regions appearing more yellow and the outer regions showing hints of red, suggestive of a range in stellar ages. Faint blue color in the outer edges suggests some degree of ongoing star formation. The object shows no apparent spiral arm structure or significant dust lanes. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major merger event.
