The galaxy presents as a somewhat elliptical structure. There is a concentrated central bulge that appears to be composed of older stellar populations, exhibiting a yellowish hue. Moving outward from the core, there is a disk-like component that presents with a more diffuse light. There are some indications of a spiral arm structure in the disk but it is not well defined. The galaxy exhibits signs of possible interaction or internal disturbance with some areas of asymmetric light distribution, potentially a minor disturbance. The overall color suggests ongoing, but perhaps not intensely vigorous, star formation. The galaxy does not appear to be undergoing a major merger, though some degree of tidal interaction cannot be ruled out entirely.
