The galaxy presents as a relatively smooth, elongated structure. Its shape is markedly cigar-like, with a central bulge that appears brighter than its outer regions. The color distribution suggests a concentration of older stellar populations in the central region, manifesting as a slightly redder hue. There is evidence of a disk, indicated by the slight bluer color gradient in the outer regions.

The lack of prominent spiral arms or distinct features indicates that star formation is not occurring at a high rate within this galaxy. There is no major signs of disturbance.