The galaxy in the image exhibits a somewhat elongated, cigar-like morphology. It displays a smooth overall appearance, with a possible indication of a disk-like structure viewed at an oblique angle. The color profile shows a shift towards the redder end of the spectrum, suggesting an older stellar population. There are some subtle color variations across the galaxy's structure, possibly indicating areas of ongoing, low-level star formation, though this is difficult to ascertain definitively from the image alone. There is no obvious evidence of major disturbances in the galaxy's morphology, suggesting it has not undergone a major merger event recently.
