The galaxy presents a predominantly smooth, elliptical morphology. Its color profile suggests an older stellar population, with a yellow-orange hue concentrated towards the center. There is an absence of prominent spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, exhibiting no obvious signs of a major ongoing merger, though subtle irregularities or faint tidal features cannot be entirely ruled out. The elongated shape indicates the galaxy is not perfectly spherical; it is somewhat cigar shaped. A slight color gradient, from a bluer periphery to a redder core, is present, suggesting some level of ongoing, though limited, star formation. The galaxy exhibits a distinct, centrally concentrated bulge.
