The galaxy presents a predominantly smooth morphology, with a high degree of circularity. There's no apparent spiral structure or distinct disk features visible. The light is concentrated towards the center, suggesting a prominent galactic bulge. The color gradient transitions from a yellowish core to a redder halo, indicative of an aging stellar population within the bulge, and potentially a low level of star formation. The outer regions appear diffuse and are difficult to resolve in detail, the image resolution is limited. There are no signs of ongoing major mergers or tidal disturbances visible. The galaxy appears to be in a relatively quiescent state.
