The galaxy presents as a somewhat elliptical, relatively smooth structure, with an apparent axis ratio of approximately 0.65. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. A slightly fainter, extended halo surrounds the core. The galaxy shows a subtle color gradient, transitioning from a yellowish-white center to a slightly bluer hue in the outer regions. There is some indication of a very subtle disk-like morphology, though it is not well defined. No prominent spiral arms or dust lanes are visible. The morphology suggests it is a mature galaxy, possibly an elliptical or lenticular type. There may be some minor disturbances but overall the structure does not appear to be actively merging with another galaxy.