The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. These arms are somewhat fragmented and display a clumpy appearance, suggesting active star formation regions. A central bulge is discernible, appearing moderately sized and yellow-ish in color, indicative of an older stellar population.

There is a noticeable bar structure spanning a significant portion of the galaxy's disk. The bar appears relatively strong.

Evidence suggests a possible ongoing or past merger event. One region of the galaxy appears disturbed or exhibits tidal features. Another region shows disruption in its structure, which could be indicative of interaction.
