The galaxy presents a mostly smooth morphology, although some features or a disk cannot be entirely ruled out. It appears elongated, with a cigar-like shape. The dominant color is yellowish-orange, concentrated towards the center, suggesting an older stellar population. There are hints of bluer regions, particularly towards one end. The presence of these bluer regions indicates potential areas of ongoing star formation. There is a smaller, bluer object near the main body, potentially a companion galaxy, a region of intense star formation, or an artifact. No signs of major mergers are apparent, but minor disturbances might be present. The smooth and elongated overall shape suggests a classification leaning towards elliptical or lenticular, but the presence of bluer regions complicates a definitive classification without further spectral data.
