The galaxy presents as a somewhat elongated, disk-like structure. It displays a relatively smooth overall appearance, although subtle features suggest the possibility of a disk. The central region appears brighter and more concentrated, possibly indicating the presence of a bulge. The color distribution shows a gradient, with a yellowish hue in the central bulge area, and more blueish and reddish tones extending towards the outer regions of the disk, with the disk region appearing greener and more elongated. The elongation suggests a classification leaning towards a cigar shape. No signs of major mergers or significant disturbances are readily apparent in the image. The galaxy likely has a moderate stellar mass, and possibly low star formation rates. The smoothness suggests that it could potentially be a disk galaxy with a significant spheroidal component.