The galaxy presents as a somewhat elliptical, diffuse structure. The central region exhibits a high degree of luminosity, suggestive of a concentrated stellar population or active galactic nucleus. Moving outward, the light gradually diminishes, with a smooth transition from the bright core to the fainter outer regions. There is very little evidence of spiral arm structure. The overall color appears slightly blue-green, hinting at the presence of younger, hotter stars. The galaxy's shape is more in between circular and elongated. There are no signs of any major merger events and appears to be a quiet galaxy.
