The galaxy presents as a relatively smooth, elliptical-like object. There is a slight elongation in the morphology, but it is mostly rounded in appearance. The galaxy has a concentration of light towards the center, suggesting a bulge. There are no apparent spiral arms or a prominent disk-like structure visible in this imaging. The color appears to be slightly redder, indicating an older stellar population. There is no evidence of any major merging or tidal disturbances; it appears to be a relatively isolated galaxy in its current state. Based on these observations, it is likely an early-type galaxy with a significant spheroidal component.
