The galaxy presents a generally smooth morphology, though it is difficult to definitively classify it as purely elliptical due to slight disk-like structure. The central region exhibits higher luminosity compared to the outer regions, indicative of a possible central bulge. There may be some disturbances. It shows a faint tidal tail on one side. The color profile suggests a population of older stars, with limited ongoing star formation. The galaxy displays a flattened shape, indicating that it has some rotation, but not very quickly, and no large spiral arms.