This galaxy exhibits a pronounced elongated, cigar-like morphology. Its light distribution appears relatively smooth and unstructured, suggesting a lack of prominent spiral arms or distinct features. The color profile indicates a predominantly red hue, implying an older stellar population with a lower rate of ongoing star formation. The galaxy's shape doesn't show any signs of major disturbances or mergers, suggesting it is a relatively isolated system. Despite the lack of prominent features, subtle color variations suggest some internal structure, possibly related to variations in stellar density or dust distribution within the galaxy. Overall, the galaxy appears to be a relatively evolved, quiescent system.
