This galaxy exhibits a flattened, disk-like morphology, viewed approximately edge-on. The central region appears brighter and more condensed, suggestive of a bulge component. The color gradient indicates a radial change in stellar populations, with the central bulge appearing yellower compared to the bluer hues observed in the outer disk. This difference could be due to higher metallicity stars or a lack of star formation in the center of the galaxy. 

Faint extensions are observed on either side of the bulge, suggesting a spiral structure or tidal arms. These are not clearly defined but appear relatively uniform. It is possible that the galaxy is in an early stage of merging with a minor companion or has experienced a minor disturbance in the past, given the slight irregularities in its overall form.