The galaxy presents as a fairly symmetrical elliptical morphology. The central bulge appears as a concentrated region of yellow-white light, indicative of an older stellar population. A surrounding, less concentrated halo extends outwards, showing hints of green, possibly indicating some ongoing, though limited, star formation in the outer regions. The overall structure is smooth and largely undisturbed, with no apparent signs of a major merger or tidal interactions. The shape appears mostly round with subtle elongation. There is a lack of distinct spiral arms or a well-defined disk structure.