The galaxy presents a generally smooth and rounded morphology. There is a concentrated central bulge exhibiting a yellowish hue, suggesting a population of older stars. Moving outwards, the galaxy appears less concentrated, with a gradual decrease in luminosity. The outer regions display a faint greenish tint. There is no obvious presence of spiral arms or a distinct disk-like structure, indicating the galaxy is likely an elliptical type. There is no evidence of any major merging activity or significant tidal disturbances.
