The galaxy presents as a relatively compact object with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, suggesting a population of older stars. Fainter, bluer extensions are visible emanating from the core region, potentially indicative of ongoing star formation within a disk-like component. There are hints of disturbances in the outer regions, possibly resulting from minor gravitational interactions or mergers. The overall structure suggests a system undergoing a transition from a relatively smooth, spheroidal form towards a disk-dominated configuration, or the aftermath of a recent merger event. The color gradients suggest a radial variation in stellar populations, with the core dominated by older, redder stars and the outskirts showing evidence of younger, bluer stars.
