The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, characterized by a bright yellowish hue, suggesting an older stellar population. Moving outward from the core, the light gradually diffuses. Some bluer tones in the outer regions hint at younger stars, suggesting some ongoing star formation. There is no clearly visible spiral arm structure or a prominent dust lane. The overall morphology appears relatively undisturbed, showing no major signs of a recent merger event, although some minor distortions are present.
