The galaxy presents a somewhat elliptical morphology, exhibiting a noticeable disk structure. The central bulge is prominent and displays a bright, yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the disk shows a blend of colors, with hints of redder regions indicative of dust lanes and potentially some ongoing star formation. However, star formation appears to be relatively subdued, with only faint blueish tinges discernable. There are no clear signs of strong spiral arms, and the overall structure appears relatively smooth, although subtle irregularities suggest minor disturbances or past interactions. The galaxy's shape shows no indications of an ongoing major merger.
