The galaxy appears to be a spiral galaxy, viewed at an oblique angle, but not quite edge-on. It presents a bright, concentrated central bulge exhibiting a yellowish hue, likely indicative of an older stellar population dominating the core. Fainter disk components extend outward, showing a bluish tinge, possibly suggestive of younger, hotter stars.

The disk reveals hints of spiral arm structure, but these features are not sharply defined. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or interactions. The color gradients suggest some ongoing star formation, but the rate is likely subdued, based on the modest blueness observed.
