The galaxy appears to be a somewhat irregular system, with a dominant central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Surrounding the bulge is a region of bluer, less defined structure, potentially indicative of ongoing star formation. This bluer region is somewhat clumpy and asymmetric, and appears to extend away from the main body of the galaxy. There is evidence of potential tidal disturbances or interactions, particularly around the outer edges of the bluer region. The overall shape is neither purely elliptical nor a well-defined spiral. Instead, it leans toward being amorphous, with a disturbed or merging appearance. It is also quite small in size.
