The galaxy presents a generally smooth and rounded morphology. There is a concentration of light towards the central region, likely a bulge component, which appears to be more red in color. Fainter, bluer light extends outward from this central region. These extensions appear irregular and do not resolve into obvious spiral arm structures. The overall profile suggests minimal disturbance from recent major mergers. The size of the galaxy indicates it is a relatively massive system. The presence of bluer light in the outer regions suggests the potential for some ongoing star formation. Overall it appears to be a large, relatively undisturbed galaxy with some star formation.
