The galaxy presents as a centrally concentrated system, appearing largely smooth with a somewhat elliptical morphology. The core region displays a brighter, yellowish-white hue, suggesting an older stellar population with lower levels of ongoing star formation. Moving outward from the core, the galaxy's color transitions to a slightly redder tone, before the light from the galaxy fades into the background. No distinct spiral arm structures or significant dust lanes are visible. The overall appearance suggests a relatively quiescent system, possibly an elliptical galaxy or a lenticular galaxy seen at an angle that obscures any potential disk features. There is no evidence of major mergers or tidal disturbances in the surrounding vicinity.
