The galaxy presents an elliptical morphology. It appears to be relatively smooth in texture and elliptical in shape, exhibiting a high degree of central concentration of light. There are no distinct spiral arms or a prominent disk structure visible. The color gradient suggests a population of older stars, contributing to its reddish-yellow hue. The galaxy also appears to be interacting gravitationally, possibly in the early stages of a minor merger. This interaction manifests as a slight asymmetry in the galaxy's outer regions. The overall angular size of the galaxy is relatively compact, indicating that it is a smaller galaxy. This suggests it could be a dwarf elliptical or a more compact elliptical galaxy.
