The galaxy presents as a roughly elliptical structure, elongated in shape with a high degree of central concentration. The light distribution appears smooth, lacking prominent spiral arms or distinct features indicative of ongoing major mergers or significant tidal disturbances. The central bulge exhibits a bright, concentrated luminosity profile, suggesting a potentially older stellar population. The outer regions of the galaxy appear less luminous and bluer in color, indicating the presence of a younger stellar population and some ongoing star formation, albeit at a relatively low rate. Overall, the galaxy appears relatively undisturbed and quiescent.
