The galaxy presents as a spiral type, though with some notable irregularities. A prominent central bulge exhibits a yellowish hue, indicative of an older stellar population. Extending from the central bulge are spiral arms, which appear somewhat disrupted and asymmetric. These arms are bluer in color compared to the bulge, suggesting the presence of younger, hotter stars and active star formation. The spiral arms show evidence of star formation activity, and potentially disturbances from past or ongoing interactions. A significant amount of disturbance can be seen in the arms, with the galaxy presenting a chaotic appearance. The galaxy appears to be undergoing or has recently undergone a merger, indicated by a disturbed morphology.
