The galaxy presents as a slightly elongated, lenticular or early-type spiral structure. It appears largely smooth in texture, with a dominant central bulge that constitutes a significant portion of its overall light output. There is some indication of a possible disk, but it is not well-defined and lacks prominent spiral arm features. The light appears to emanate more strongly in the blue, or green bands, with less light in the red. Given the bluer color profile and moderate luminosity, the galaxy likely has a moderate rate of star formation. There is an indication of minor disturbances in the morphology, potentially from a minor interaction or accretion event, but no ongoing merging is immediately apparent. Overall, the galaxy seems to be relatively isolated and mature in its evolution.
