The galaxy presents as an elliptical system with an apparent smooth morphology. The central region exhibits a high degree of luminosity, appearing yellowish, suggesting an older stellar population. This bright central bulge gradually fades into a surrounding disk. The disk structure is subtle, with faint blue hints indicating the presence of younger stars and potential ongoing star formation regions. The shape appears elongated, with a roughly elliptical form. There is a minor asymmetry in the outer regions, potentially indicative of a past or ongoing interaction.
