The galaxy presents a compact morphology with a bright, concentrated core. The light distribution appears relatively smooth, lacking distinct spiral arm structures or a prominent bulge. There is a faint, diffuse halo surrounding the core, exhibiting a slightly irregular shape. It looks disturbed with some interaction or merging occurring. There is a second possible galactic center in the diffuse light. The galaxy exhibits a blue-ish hue, suggesting a potentially active star formation rate or a population of young, hot stars within the system.
