The galaxy presents as a somewhat elliptical structure with a high degree of central concentration. The light profile suggests a bulge-dominated system, with the majority of the luminosity concentrated towards the galactic center. The color of the central region appears slightly redder or yellower than the outer regions, which is potentially indicative of an older stellar population or a higher dust content in the core. The galaxy does not exhibit strong spiral arm features or any obvious signs of recent major merger activity; however, there are some faint asymmetries or irregularities in its outer halo that could suggest minor interactions or disturbances. Overall, the object appears relatively smooth in appearance.
