The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a discernible core that appears bright, gradually diffusing outward. The central region presents a yellowish white color, which suggests an older stellar population. The outer regions of the galaxy show hints of a redder hue, possibly indicating a lower rate of recent star formation. There are no apparent spiral arms, strong dust lanes, or other distinct features such as tidal tails or distorted morphology. This suggests that the galaxy may be an elliptical galaxy.
