The galaxy presents as a roughly elliptical structure with a smooth, diffuse light distribution. There is a central, brighter region suggesting a concentration of stars or potentially an active galactic nucleus. The overall color appears relatively blue-white, hinting at a population of younger, hotter stars. The outer regions fade gradually into the background, with no distinct spiral arms or prominent dust lanes visible. The morphology suggests a relatively evolved system with little ongoing major star formation based on the lack of significant features or disturbances. There is some indication of a very slight tidal disturbance, but overall, the galaxy appears relaxed.
