The galaxy presents a largely smooth, rounded morphology. The primary light distribution is concentrated in a central bulge, appearing approximately spherical. There is a subtle color gradient, with the core exhibiting a yellower hue, suggesting a population of older stars. Faint extensions of diffuse light are barely visible, indicating a possible, very subdued disk-like component or stellar halo, but no distinct spiral arm structures are apparent. Based on its color and morphology, it is potentially an elliptical galaxy or a lenticular galaxy with a prominent bulge. There are barely noticeable irregularities, which may indicate minimal ongoing or recent merger activity.
