The galaxy appears as a relatively compact object. The dominant color is a vibrant blue-white, suggesting a significant population of young, hot stars. The central region exhibits a high concentration of luminosity, possibly indicating an active galactic nucleus or a dense stellar population. The overall structure appears largely spheroidal with little, if any, discernible spiral arm structure or prominent disk. The outer edges fade gradually, indicating a smooth density gradient. There is no obvious signs of major tidal disturbances or ongoing mergers, however, there seems to be very slight asymmetric distribution of light, suggesting possible minor interaction or internal dynamics influencing its shape. The galaxy's appearance is largely smooth and relatively featureless.
