The galaxy presents as a diffuse, elliptical-like structure with a bright, concentrated core. The main body appears relatively smooth, lacking prominent spiral arms or distinct features. The color profile suggests the presence of an older stellar population, with a possible contribution from intermediate-age stars. The light distribution from the central region fades gradually outward, indicating a high Sersic index. A slight flattening of the galaxy is observed, with the major axis oriented approximately north-northwest to south-southeast. There is visual evidence of potential disturbances to the galaxy's morphology.
