This galaxy presents as a system with a dominant central bulge. The bulge exhibits a yellow-orange hue, suggesting an older stellar population. A faint, disk-like structure surrounds the bulge. This disk shows hints of spiral arms. These arms have a bluer tint, suggestive of the presence of some younger, hotter stars undergoing active star formation. There are no signs of any major mergers or tidal disturbances. Overall, the galaxy exhibits a relatively smooth structure, though not perfectly elliptical.
