The galaxy appears to be elliptical in morphology, with a smooth, diffuse light distribution. It presents a concentrated central bulge exhibiting a yellowish-orange hue, indicative of an older stellar population. The outer regions of the galaxy exhibit a bluer color, suggesting the presence of some younger stars or ongoing star formation, though limited. There is no apparent spiral structure or bar. The galaxy does not appear to be undergoing any major interactions or disturbances, although there might be some minor irregularities.
