The galaxy presents as a concentrated, elliptical-like structure. It exhibits a smooth, diffuse morphology with a prominent central bulge. The core appears bright and concentrated, possibly indicating the presence of an active galactic nucleus or a high density of stars. The color profile suggests an older stellar population, dominated by redder hues in the central regions, which gradually fade to a bluish color on the outer edges, indicating possible younger stars forming on the outer fringes of the galaxy. There is no discernible spiral arm structure, nor any evidence of significant tidal disturbances or ongoing major mergers. The overall appearance suggests a relatively relaxed and evolved system.
