The galaxy presents a largely smooth morphology, exhibiting a dominant central bulge. The overall shape appears close to circular, with little deviation toward an elongated or cigar-like form. A slight disk-like structure is potentially present. Evidence for significant tidal disturbances, major mergers, or strongly interacting companions is minimal. Some visual artifacts may be present. The galaxy displays a distinctive color profile, with bluer emission concentrated in the central regions and transitioning to redder hues in the outer areas. This suggests a difference in stellar population, with possible ongoing star formation in the inner area.
