The galaxy presents as a primarily smooth, centrally concentrated object, exhibiting a moderate degree of roundness. There is a slight asymmetry to its shape, suggesting a possible minor disturbance or interaction. The central region appears brighter and more yellow/orange in color than the outer regions, which fade to a less saturated hue. The overall color suggests an older stellar population. No distinct spiral arms or bar structures are discernible. The object does not appear to be undergoing a major merger, although the slight asymmetry might indicate a past or ongoing minor interaction with a smaller object.
