The galaxy presents a mostly smooth morphology, with a slight disklike appearance suggesting it is not entirely spheroidal. There is some indication of disruption, possibly due to a minor interaction or merger event. The galaxy appears relatively compact, approximately 7.5 kpc across, and exhibits a central concentration of light that is yellowish-red in color. This color suggests a population of older stars. The presence of bluer regions hint at ongoing, though subdued, star formation in certain areas. Overall, the galaxy appears to be a moderately massive system in a transition stage, perhaps evolving from a more actively star-forming state to a quiescent one.
