The galaxy presents as a slightly elongated, centrally concentrated system. The light distribution appears relatively smooth and diffuse, suggesting a lack of prominent spiral arm structures or distinct clumps of star formation. The central region exhibits a brighter, more condensed core, likely indicating a bulge component. There is a subtle color gradient from the center outwards, with the core appearing slightly more yellow/white, transitioning to a bluer hue in the outer regions. There are hints of possible slight disturbance or tidal features, but they are faint and do not dominate the overall morphology. The galaxy appears to be a relatively evolved system with ongoing, but possibly subdued, star formation. The overall shape is neither perfectly spherical nor highly flattened, occupying an intermediate morphology.
