The galaxy presents a primarily smooth, somewhat elliptical morphology. A bright central bulge dominates the structure, surrounded by a less defined, fainter halo of stars. Evidence suggests the presence of potential tidal disturbances or faint spiral arm segments that could indicate past or ongoing interactions. These disturbances are visible as subtle, elongated extensions of the galaxy's outer regions, showing hints of asymmetric features. The color distribution indicates a central concentration of older stellar populations, surrounded by regions exhibiting bluer, potentially younger stars, especially in the areas possibly related to tidal features. Overall, this galaxy appears to be in a transitional state, likely undergoing a slow merging or interaction process.
