The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The overall color is a dominant yellowish-red hue, suggesting an older stellar population. The galaxy appears approximately round, with a slight elongation that could be due to a mild disk structure, though this is not clearly discernible. There is a very subtle hint of a slight disturbance or asymmetry, possibly indicating a minor gravitational interaction. Overall, the galaxy's morphology suggests a quiescent state with minimal ongoing star formation. The central concentration appears brighter than the surrounding halo.
