The galaxy presents as a moderately luminous object with a disturbed morphology, indicative of a possible interaction or recent merger event. A central, somewhat condensed region emits primarily in the green and blue wavelengths, suggesting active star formation. There are areas that emit at redder wavelengths. The galaxy does not exhibit a highly symmetrical or well-defined spiral structure. There are notable disturbances in its morphology. There appears to be a minor companion galaxy, or tidal tail structure present in the upper right, further supporting the hypothesis of an interaction. Overall, the galaxy displays a moderate degree of ongoing star formation activity and morphological disturbance.
