The galaxy presents as a primarily smooth, elliptical-like structure. The core region exhibits a concentrated luminosity, appearing almost spheroidal. The light distribution graduates outwards, diminishing in intensity from the central region. There may be a slight hint of a disk, though the smoothness is dominant. The color gradients suggest a relatively evolved stellar population, with redder hues predominating. There is no strong evidence of active star formation regions or prominent spiral arms. The overall morphology suggests a system with a high degree of symmetry. Close inspection does not indicate major mergers or significant tidal disturbances; however, minor irregularities cannot be excluded at this resolution.
