The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth, relatively featureless appearance, suggesting it is likely an early-type galaxy. There is no evidence of spiral arms or a prominent disk structure. The light distribution shows a strong radial gradient, with the brightest region located at the nucleus, fading gradually outwards. The galaxy is not perfectly circular; instead, it appears slightly elongated, tending towards an oblate spheroid shape. No significant tidal features, distortions, or signs of recent merging activity are observed in the immediate vicinity. The color profile appears generally uniform across the galaxy, indicating a relatively homogeneous stellar population.