The galaxy presents as a moderately sized, elliptical-like structure with a smooth overall appearance. Its color profile indicates a composition of primarily older stellar populations, as evidenced by the redder hues concentrated within the central bulge and the surrounding halo. The galaxy appears mostly undisturbed, showing no strong signs of recent major mergers, although some slight asymmetry in its morphology might suggest a past minor interaction. The overall form is somewhat elongated but primarily rounded, with a high central concentration of light gradually fading towards the outer edges. There is some indication of possible low-level star formation, with subtle blue tinges noted in small and isolated patches, suggesting limited ongoing activity. 
