The galaxy presents as a generally smooth, elliptical structure. It exhibits a concentrated, bright central bulge that gradually fades into a less luminous, more diffuse halo. The overall shape appears to be somewhat elongated rather than perfectly spherical. There may be subtle indications of a disk component but it's very faint. There is no obvious evidence of any major merger events or significant tidal disturbances. Color gradients suggest a variation in stellar populations or dust content from the core to the outer regions, trending towards redder hues in the center.
