The galaxy presents an elliptical morphology, appearing mostly smooth in structure with a high degree of central concentration. The galaxy's shape is elongated, with a cigar-shaped appearance. There are no obvious spiral arms or a prominent disk. The color gradient suggests a redder core, likely composed of older stellar populations, transitioning to slightly bluer hues in the outer regions, potentially indicating some ongoing, though modest, star formation. There is no evidence of strong tidal features, ongoing mergers, or significant disturbances in its morphology. The overall structure is consistent with a relatively undisturbed system.
