The galaxy presents as a somewhat smooth, elliptical-like structure, though not perfectly round. The color profile indicates an older stellar population, exhibiting a yellowish central bulge that diffuses outwards. There is a hint of a bluer component in the outer regions, suggesting some ongoing or recent star formation. No prominent spiral arms or bars are discernible. There are also some minor disturbances in the outer regions of the galaxy that could indicate it is merging. The galaxy appears to be relatively isolated with no other companions in sight.
