The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits a slightly elliptical morphology, appearing more rounded than elongated. The core of the galaxy displays a bright, concentrated luminosity, suggesting a dense stellar population in the central bulge. Moving outward from the core, the light intensity gradually diminishes, with a fainter, more diffuse halo surrounding the central region. There may be some minor asymmetry in the outer regions, hinting at possible interactions or disturbances but not a full on merger. Overall the galaxy appears relatively undisturbed.
