The galaxy presents as a centrally concentrated system with a flattened, elongated morphology. The light distribution suggests a relatively smooth structure, with no prominent spiral arms or irregular features readily discernible. There is a distinct color gradient from the central region to the outer halo, with the core appearing more yellowish, suggesting an older stellar population. The outer regions exhibit a bluer hue, potentially indicative of ongoing star formation, though at a modest rate. Overall, the galaxy appears relatively undisturbed, lacking any obvious signs of recent major merger events. Its shape deviates noticeably from being circular, leaning toward a more cigar-like structure.
