The galaxy presents an overall elliptical morphology, although a degree of disk-like structure may be present. The central region exhibits a high concentration of light, appearing bright and relatively smooth with a yellowish hue. Moving outward from the core, the galaxy becomes less concentrated, displaying a more diffuse appearance. Faint blue regions may indicate areas of star formation. There are slight indications of potential tidal disturbance or minor interaction, with some asymmetry in the outer regions, though this is not definitive. The galaxy is neither perfectly round, nor obviously elongated; appearing somewhere in between. It is of a significant mass, but has a relatively low star formation rate. 
