The galaxy presents a largely smooth, elliptical morphology. It appears to be relatively concentrated, exhibiting a fairly symmetrical, round shape with minimal discernible features. There's a slight elongation visible, but it isn't overly pronounced. The central region appears brighter and more concentrated, indicative of a significant concentration of stars towards the galactic core. Color gradients are subtle, with a general trend towards redder hues, suggesting an older stellar population and a cessation of significant star formation activity. No spiral arm structures, dust lanes, or signs of recent major mergers are apparent. There might be some very subtle asymmetries or minor disturbances hinting at potential past interactions, but overall, the galaxy appears relatively undisturbed and relaxed. The lack of prominent blue regions suggests a low rate of ongoing star formation.
