The galaxy presents as a generally smooth, elliptical-like structure, with a high degree of central concentration of light. The color profile suggests a population of older stars, visible by the yellow-red hue, with very little evidence of dust lanes or spiral arm structures. The galaxy appears roughly spherical in shape, with a soft, diffused edge suggesting a gradual decrease in stellar density toward the outer regions. There is no noticeable sign of recent or ongoing major mergers or tidal disturbances, though some faint asymmetries could suggest minor past interactions. The overall morphology is consistent with that of a quiescent, massive galaxy.
