The galaxy exhibits an elliptical morphology, appearing mostly smooth and featureless. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population. The overall shape is moderately elongated. There may be subtle color gradients, with a slight bluish tint towards the outer regions, potentially indicating some ongoing star formation, but the galaxy is primarily composed of older stars. No spiral arm structure is visible, and there is no evidence of significant dust lanes or morphological disturbances. The galaxy appears relatively isolated and undisturbed.
