The galaxy presents a predominantly smooth morphology, indicating a lack of prominent spiral arms or distinct features. It exhibits a slightly elliptical shape, appearing neither perfectly circular nor elongated. A subtle color gradient is observed across the galaxy, transitioning from a bluer hue in the central region to redder tones in the outer areas. This suggests a centrally concentrated area of ongoing star formation with older stellar populations dominating the galaxy's outskirts. There is no indication of major merger activity, although the galaxy may exhibit some minor disturbances or tidal features suggesting possible past interactions or internal dynamics. Overall, the galaxy appears to be a relatively quiescent system.
