The galaxy presents as a luminous, centrally concentrated object. The core region displays a notably smooth texture and a yellowish-orange hue, suggesting a population of older stars. Extending outward from the core is a fainter, more diffuse halo with a slight bluish tint, which might indicate regions of more recent star formation activity. The overall morphology is somewhat elongated, leaning towards an elliptical shape, though not perfectly symmetrical. There is subtle evidence of a minor perturbation or irregularity in the outer halo on the right side. The structure appears relatively undisturbed, indicating it is likely not undergoing a major merger.
