The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. The core region exhibits a yellowish hue, suggesting an older stellar population. Moving outwards from the center, the light becomes more diffuse and slightly bluer in color, potentially indicating some level of ongoing, though limited, star formation in the outer regions. There is no distinct spiral arm structure evident. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of a major merger event. However, there may be slight irregularities present in the outer regions, possibly indicating a past or ongoing minor interaction or disturbance. The galaxy is relatively massive. The inferred size of the galaxy is significant, indicating a substantial physical extent.
