The galaxy appears to be a luminous object with a central bulge, exhibiting a yellowish hue indicative of an older stellar population. There is an indication of a disk-like structure, with some asymmetric features. A bluer region to one side suggests some level of active star formation, possibly along a spiral arm or in a region of ongoing interaction. A strong disturbance indicates a possibility of a significant merger event. Overall the galaxy presents a mix of evolved and actively forming stellar populations, with signs of morphological disturbance hinting at interaction or recent merger activity.
