The galaxy presents a generally smooth and rounded morphology. It is characterized by a concentrated central bulge, which is noticeably bright and exhibits a yellowish hue, suggesting a population of older stars. There's a faint, diffuse halo surrounding the central region, extending outwards with a subtle gradient in brightness. The overall shape is relatively elliptical, with a lack of distinct spiral arm structures or significant irregularities. There is no indication of active merging or major disturbances in the galaxy's structure. The color profile suggests a dominant population of older stars.
