The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish-white hue, indicating a population of older stars. Moving outward from the core, the galaxy displays a gradual color shift towards a bluer and greener tint. This suggests the presence of a younger stellar population and potential regions of ongoing star formation in the outer regions of the galaxy. 

A subtle asymmetry is observed, with a faint extended feature on one side. There is a small, compact object, possibly a star cluster or dwarf galaxy, located adjacent to the galaxy. The overall appearance is consistent with a system that may have experienced, or is currently undergoing, minor interaction or disturbance. The galaxy does not exhibit the strong features of a spiral structure or a highly disturbed merger.
