The galaxy presents as a relatively compact object with a slightly irregular morphology. It appears to have a central, moderately bright core. Extending outwards from the core is what appears to be a disturbed disk structure, exhibiting hints of faint spiral arms or tidal features. The overall color suggests a mix of stellar populations, with bluer regions indicating recent or ongoing star formation and redder regions suggesting older stellar populations. Some dust lanes or patches of obscuration are likely present, contributing to the galaxy's irregular appearance and varied color distribution. Evidence of potential minor interaction or a past merger event can be seen from faint asymmetry/disturbance.
