The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of light concentration, appearing as a bright, yellowish core, suggesting a substantial population of older stars. The light gradually diffuses outward, forming a less distinct, somewhat fainter halo that lacks any obvious spiral arm structures or significant dust lane features. The overall color profile indicates a relatively quiescent galaxy with a low star formation rate. There is no visually apparent ongoing merger activity or significant tidal disturbances.
