The galaxy presents as a centrally concentrated object with a generally smooth morphology, though subtle features are discernable. A bright central region is visible, potentially indicative of a substantial galactic nucleus. The overall shape appears somewhat elliptical, though not perfectly so; the galaxy is closer to round than cigar-shaped. There is a hint of a disk-like structure or arm-like features emanating from the core. There are no obvious signs of a major merger or significant tidal disruption. The object displays a faint and diffuse outer halo. Color gradients are observable, the central region appearing more yellow-white, suggestive of an older stellar population, and the faint outer regions having a slightly bluer tinge which may be due to on-going star formation or a population of younger stars.
