The galaxy presents as a somewhat elliptical structure with a noticeable central bulge, appearing brighter and more concentrated than the surrounding disk. There's an indication of some disc-like structure. The light distribution is not perfectly smooth. There may be slight disturbances in the morphology. Color gradients suggest a diverse stellar population. The redder hues concentrated in the central bulge indicate older stars, while bluer regions outside the bulge suggest younger stellar populations and potentially ongoing star formation.
