The galaxy presents as a luminous, centrally concentrated spheroid. Its overall structure appears largely smooth, with a high degree of rotational symmetry, suggesting an elliptical morphology. The core exhibits a pronounced yellow hue. This potentially indicates a dominant population of older stars, with relatively low levels of ongoing star formation. Fainter, diffuse blue components suggest a small amount of recent star formation in its outer regions. Based on the apparent color profile, the galaxy's stellar population is likely dominated by evolved stars. There is no obvious evidence of a spiral arm structure or prominent dust lanes. No significant merger activity is apparent.
