The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. A central, bright region indicative of a high stellar density is apparent, gradually fading into the outer regions. There is a hint of a slight disk-like structure but it is not a prominent feature. Faint, diffuse outer regions extend beyond the central body, suggesting a halo of older stars and possibly some tidal debris. There is no strong indication of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no clear signs of ongoing major mergers, although minor asymmetries or disturbances cannot be entirely ruled out. The color gradient, from a more yellow/orange center to slightly bluer outer regions, implies variations in stellar populations, possibly indicating ongoing, yet low level, star formation in the outer regions.
