The galaxy presents a largely smooth, elliptical morphology. It appears to be a relatively undisturbed system, lacking prominent spiral arms or significant tidal features indicative of a recent major merger. The galaxy's light distribution is centrally concentrated, exhibiting a bright core that gradually fades towards the outer regions. There is evidence of color variation across the galaxy's body, with a suggestion of a slightly bluer central region transitioning to redder hues in the outskirts, possibly indicating a difference in stellar populations or dust content between the core and the outer halo. The galaxy's shape is generally round, with only a slight deviation towards an elongated, cigar-like shape.
