The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile. A dominant central bulge is apparent, characterized by a yellowish hue suggesting an older stellar population. Faint extensions emanate from the central region, potentially indicating tidal features or remnants of a past merger event. A bluer region is visible adjacent to the central structure, potentially suggesting regions of ongoing or recent star formation. Overall, the galaxy exhibits signs of interaction or disturbance in its morphology.
