The galaxy presents as a moderately bright, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish-white hue, indicative of an older stellar population. Moving outward from the center, the light gradually diminishes, transitioning to a more diffuse halo that extends in an oval shape. There is a subtle bluish tinge present in the outer regions, which could suggest some ongoing star formation. The overall form appears relatively smooth, without any clear signs of significant spiral arm structures or major disturbances. It seems to be an intermediate-sized galaxy, characterized by a generally relaxed morphology. There is a possible, minor distortion or asymmetry in the outer reaches of the galaxy. It is difficult to see any evidence of tidal tails or other signs of an ongoing merger, however there may be a minor disturbance.
