The galaxy presents a generally smooth and concentrated morphology. It appears elliptical in shape, exhibiting a high degree of radial symmetry. The light profile increases towards the center, displaying a strong central bulge that transitions to a more diffuse halo or outskirts. Color gradients suggest an aging stellar population, with redder hues concentrated towards the core. There is minimal evidence of spiral arm structure or significant dust lanes. There is no apparent nuclear activity, based on the lack of a bright, point-like source at the galaxy's center. Overall, the galaxy appears to be a mature system, likely dominated by older stars and quiescent star formation.
