The galaxy exhibits a generally smooth morphology with minimal discernible features such as spiral arms or a prominent disk. Its shape appears close to round with a hint of elongation. The galaxy displays a color gradient, transitioning from a brighter, more centrally concentrated region towards a fainter outer halo. The light distribution suggests a relatively smooth and centrally concentrated stellar population. There are no obvious signs of recent major merging events or significant tidal disturbances, although subtle asymmetries cannot be entirely ruled out. Overall, the galaxy presents as a relatively undisturbed system dominated by an older stellar population with moderate star formation activity.
