The galaxy presents as a relatively smooth, elliptical-like structure. A central bulge region exhibits a concentrated, bright intensity with a yellowish hue. The surrounding halo gradually diffuses outwards, transitioning in color to a faint bluish tint, particularly at the outer edges, suggesting the presence of a younger stellar population than the bulge. There are no prominent spiral arms, bars, or other distinct features visible, and its shape is more in between of round and elliptical. There may be a minor interaction or disturbance evident.
