The galaxy appears as a relatively compact object with a centrally concentrated light profile, suggestive of an elliptical galaxy. The central region exhibits a bright, yellowish hue, potentially indicating an older stellar population. The overall morphology appears largely smooth, with no prominent spiral arms or distinct features visible. There is a subtle color gradient moving outwards from the core. The galaxy seems relatively isolated with no signs of major tidal disturbances or active merging events. A small amount of blue light is visible, which could indicate some recent star formation, though at a very low rate. The overall shape appears mostly circular, with only a very slight elongation, if any.
