The galaxy presents as a somewhat diffuse, elliptical object. A brighter central region is apparent, possibly indicating a core or nucleus. While a defined disk structure is not immediately obvious, the overall morphology does not appear entirely smooth, suggesting the presence of some internal structure. The color gradient implies a variation in stellar populations or dust content across the galaxy, where the outer regions appear less red. There is a possible indication of minor disturbance in its morphology, perhaps a faint tidal feature, but this requires closer inspection. The galaxy does not appear to be undergoing a major merger.
