The galaxy presents a primarily smooth, elliptical morphology. It appears well-rounded, exhibiting a high degree of radial symmetry. The galaxy's light distribution is concentrated towards its center, suggesting a prominent bulge component. There are some subtle color variations within the galaxy, with a slightly redder hue near the center that gradually transitions to a bluer periphery. This color gradient could indicate differences in stellar populations or dust content between the galaxy's core and outer regions. No distinct spiral arms or bar features are readily apparent; it is mainly a centrally condensed object. There is no evidence of any major merger events or significant tidal disturbances in its surrounding environment. However, there's the suggestion of a minor asymmetry, potentially indicating past or ongoing interactions.
