The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a generally smooth and featureless morphology. There is a slightly elongated shape, not perfectly spherical, with a smooth gradient of light intensity emanating from a bright central bulge region. The color profile suggests an older stellar population, particularly within the core, where the light appears redder. Fainter blue light surrounds this core suggesting a bit of younger star formation compared to the core. There is no evidence of spiral arms or a prominent disk structure. There is no obvious interaction or disturbance from other nearby objects. The general characteristics seem consistent with a galaxy that has undergone significant evolution and is currently relatively quiescent in terms of star formation activity, although there may be some ongoing formation, specifically in the areas surrounding the core.
