The galaxy presents as a generally smooth, elliptical-like structure, with a slight elongation. There is a subtle color gradient, transitioning from a more yellowish hue towards the center to a bluer tinge in the outer regions. The central region appears more concentrated and luminous. There is no obvious spiral arm structure or prominent dust lanes visible at this resolution, suggesting a lack of significant ongoing star formation. No signs of major mergers or tidal disturbances are apparent; the galaxy appears relatively undisturbed. The overall morphology points to a galaxy with an evolved stellar population.
