The galaxy presents a somewhat elliptical morphology, appearing largely smooth in structure. Its central region exhibits a concentrated, bright luminosity, suggestive of a significant stellar population. Moving outward from the core, the luminosity gradually decreases. The outer regions show a subtle disk-like structure, though no distinct spiral arms are discernible. The galaxy's overall color is a slightly off white hue. There's no evidence of a major merger event disrupting the main structure, though there might be very slight indications of minor disturbances in the outer halo. Overall, the galaxy appears to be a relatively undisturbed, evolved system with a likely ongoing, but moderate rate of star formation.
