The galaxy presents as a moderately bright, elliptical-like structure. Its core exhibits a concentrated luminosity, appearing almost spheroidal in shape. Moving outward, the galaxy diffuses into a more elongated form, indicating a departure from perfect roundness. The overall color profile suggests a relatively older stellar population, with subtle hints of blue possibly indicating regions of recent star formation. There are no apparent spiral arm structures, and the galaxy appears largely undisturbed, without significant signs of tidal interactions or major mergers. The morphology is generally smooth, with a slight asymmetry hinting at a minor interaction in its past.
