The galaxy exhibits a generally elliptical morphology with a bright, concentrated core region. The light profile appears smooth, lacking prominent spiral arm structures. The core region displays a yellowish-white hue, indicative of an older stellar population dominating the central bulge. Moving outwards from the core, the galaxy's light gradually diffuses, becoming fainter and slightly bluer in color, suggesting the presence of a younger stellar population in the outer regions, although the overall star formation activity appears to be relatively low. There is a slight asymmetry in the outer regions with a minor disturbance evident to the lower right of the core. There is no prominent dust lane or strong indication of a recent major merger event. The general characteristics suggest an early-type galaxy, potentially an elliptical or lenticular galaxy viewed from a relatively face-on perspective.
