The galaxy presents as a single, fairly compact object with a dominant bulge component. It exhibits a smooth, elliptical morphology, appearing largely undisturbed. The light distribution is centrally concentrated, with a noticeable color gradient, shifting from a bright, yellowish core to a slightly bluer outer halo or disk. There are no obvious signs of spiral arms or distinct features within the halo, though the object is somewhat blurry. This suggests a relatively old stellar population and a low ongoing star formation rate within the observed region. The core's color indicates a higher concentration of older stars.