The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated luminosity profile. The core region is bright and appears to be comprised of older stellar populations, indicated by the yellow-red hue. Moving outward from the core, the light intensity gradually decreases, exhibiting a smooth transition. Some blue is visible at the outer parts of the galaxy, indicating pockets of younger stars. There is no obvious disk structure or spiral arm features. No major disturbances or tidal tails are apparent, suggesting it is not undergoing any major merger events. The galaxy appears relatively undisturbed.
