The galaxy presents as a somewhat smooth, elliptical object. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the galactic nucleus. The luminosity gradually decreases from the core outwards, forming a diffuse halo. The overall shape is elongated, appearing more cigar-shaped than circular. There may be a slight asymmetry in the outer regions, but no obvious signs of major disturbances or ongoing mergers are apparent. Faint color variations are detectable, with a hint of redder hues in the central bulge and bluer tones towards the outskirts. The galaxy appears relatively isolated, without any immediate close companions that might indicate a recent or ongoing interaction.
