The galaxy presents as a relatively smooth, rounded object. Its overall color profile suggests a galaxy dominated by older stellar populations, exhibiting a yellowish-white hue in its central region. There is a slight elongation in its morphology, but it's generally quite symmetrical. No distinct spiral arms or prominent dust lanes are discernible. There is no evidence of strong tidal features or major merger events. The galaxy's structure indicates a likely elliptical or lenticular classification, with little to no ongoing star formation readily apparent.
