The galaxy presents a generally smooth morphology, appearing somewhat elliptical in shape. The central region exhibits a higher concentration of light, suggesting the presence of a galactic bulge. The color profile indicates a dominance of older stellar populations in the central regions, with a yellowish-orange hue. Moving outwards from the center, a subtle shift towards bluer tones can be observed, hinting at the presence of younger, hotter stars in the outer regions, potentially within a disk component. The overall structure shows no strong evidence of spiral arms or significant dust lanes, implying it could be a relatively evolved system. There are signs of minor disturbances in the galaxy, indicating that it might have undergone minor interactions or mergers in the past. The smooth, round-like shape could indicate that the galaxy is in the earlier stage of its evolution.
