The galaxy presents as a moderately inclined disk system. It exhibits a prominent, centrally concentrated bulge that appears smooth and featureless. The disk component shows a degree of asymmetry, potentially indicative of tidal interactions or internal dynamics. The color profile suggests an older stellar population dominating the bulge, with a gradual shift towards bluer colors in the outer disk, hinting at more recent star formation activity in these regions. The overall morphology is consistent with an early-type spiral galaxy, possibly undergoing a transition. There is some indication of a faint stellar halo extending beyond the main disk, though its structure is poorly resolved in this image.