The galaxy presents as a relatively compact, luminous object. There appears to be a central concentration of light that is orange/yellow in color. There are several distinct concentrations of stars. The system shows some indication of disturbance in its morphology, possibly due to a recent or ongoing interaction or merger. The disk appears perturbed, with some asymmetry evident. There's also no clearly defined spiral structure, which could indicate a lack of well-defined arms or that the galaxy is in the process of merging, disrupting its morphology. The overall color indicates a population that includes older stars, alongside some evidence of ongoing or recent star formation as indicated by the bluer star-forming regions.
