The galaxy presents as a relatively compact object, likely a lenticular or early-type spiral galaxy based on its smooth, elliptical morphology. Its central bulge appears prominent, and its overall structure demonstrates a high degree of radial symmetry. Faint, diffuse light extends outward from the core region but no distinct spiral arm structures or dust lanes are discernible. The galaxy is characterized by a smooth, featureless appearance. Its color profile suggests it consists primarily of an older stellar population, consistent with suppressed star formation activity. The shape is more rounded than cigar shaped. There are no merging features.
