The galaxy presents as a generally smooth and rounded structure. There is a distinct color gradient, with a central core exhibiting a warmer, yellower hue, likely indicating a higher concentration of older stellar populations. The outer regions display a cooler, bluer color, suggestive of ongoing or recent star formation, though it appears subdued. No prominent spiral arms, bars, or other distinct features are readily apparent. Minor disturbances, such as tidal tails or distorted morphology, are not observed. Overall, the galaxy appears relatively undisturbed and quiescent in its morphology.
