The galaxy appears as a centrally concentrated, somewhat smooth object. It has a roughly elliptical morphology and exhibits a gradual decrease in luminosity from the core outwards. The color is predominantly a pale blue-white, suggesting a population of relatively young, hot stars. The galaxy lacks any obvious spiral arm structures or dust lanes, instead exhibiting a diffuse, even light distribution. There are no obvious signs of major mergers or tidal disturbances. Based on its apparent smoothness and color profile, the galaxy could be classified as an early-type galaxy, possibly an elliptical or lenticular galaxy.
