The galaxy presents as a moderately luminous system, exhibiting a predominantly smooth morphology. It appears elliptical in shape, though not perfectly spherical, with a slight elongation. The central region displays a bright, concentrated core, suggesting a high density of stars. Moving outward from the core, the luminosity gradually decreases, indicating a declining stellar density. There are hints of some faint features or minor disturbances in the outer regions of the galaxy. There does not appear to be strong spiral arm structure or a prominent disk component. The color profile suggests an intermediate stellar population. The system exhibits a weak rate of star formation. Overall, it appears as an evolved galaxy, possibly in the process of settling towards a redder color.
