The galaxy presents as a somewhat compact, centrally concentrated object. The core region exhibits a distinct bluish-white hue, indicative of potentially younger stellar populations or active galactic nuclei activity. There is a fuzzy or diffuse, extended halo of lighter blue light surrounding the central region. The galaxy's overall shape appears relatively smooth, though there's a subtle, irregular extension towards the bottom, marked by a yellow/orange shift in color. This asymmetry suggests the possibility of a minor tidal interaction or ongoing merger event. The lack of well-defined spiral arms or a prominent disk points towards an elliptical or lenticular morphology, though a precise classification requires higher resolution imaging. The color gradient from the core outwards suggests differing stellar populations and/or dust distributions within the galaxy.
