The galaxy presents a generally smooth, rounded morphology. It displays a concentrated central region that diminishes gradually outward with no obvious spiral arm structures or a prominent disk. There are hints of minor irregularities or a slight disturbance in the galaxy's outer regions, but these are not significant enough to categorize the galaxy as undergoing a major merger or interaction. The shape appears mostly round. The colour of the galaxy is largely a consistent hue, showing no evidence of strong colour gradients or distinct colour regions suggesting any ongoing merger or interaction. Overall, the light profile suggests a centrally concentrated galaxy with some possible minor disturbance.
