The galaxy presents as a relatively compact and concentrated object with an apparent smooth morphology. Its overall shape appears round. There is no obvious spiral structure or distinct disk component visible; the light is concentrated towards the center. The color profile suggests a central region that is more yellow-white, possibly indicating an older stellar population. Surrounding this is a bluish halo, which could be indicative of younger stars. The outer regions exhibit a gradual decline in luminosity. No signs of ongoing major mergers or tidal disturbances are clearly discernible. The object displays a fairly uniform structure, with no significant irregularities or features that would strongly indicate recent interactions.
