The galaxy presents a generally elliptical morphology, with a smooth, diffuse appearance. The color profile suggests a relatively evolved stellar population, with a concentration of older, redder stars towards the galactic center. There is faint evidence of bluer, possibly younger stars in the outer regions, implying some low-level ongoing star formation. The galaxy is largely undisturbed, showing no significant tidal features or signs of a major merger event. There is slight irregularity to the shape of the galaxy, suggesting a possible minor disturbance.
