The galaxy presents a primarily smooth morphology, with a highly concentrated central bulge that appears near-spherical. The color of the core region is notably yellowish-white, suggesting a population of older stars. There is a hint of a potential disk structure surrounding the central bulge, exhibiting a slight elongation. The overall color of the disk appears more reddish than the core, which could indicate older stellar populations or dust extinction. There appears to be a tidal tail or minor disturbance present in the galaxy's morphology to the lower right of the core. Overall, the galaxy presents a high degree of light concentration.
