The galaxy appears to be an elongated, elliptical system. It presents with a smooth, featureless morphology in the visible light spectrum, indicating a lack of prominent spiral arms or significant dust lanes. The central region exhibits a higher concentration of light, suggesting a dense galactic nucleus. The overall color is skewed towards the redder end, potentially indicating an older stellar population dominated by red giant stars and a lower rate of ongoing star formation within the galaxy. The aspect ratio suggests a possible cigar shape when viewed from our current angle. There are hints of minor disturbances or asymmetries, but the galaxy seems to be relatively undisturbed, without significant signs of an ongoing merger.
