This galaxy presents a mostly smooth, disc-like morphology. A bright central bulge dominates the galaxy's structure, displaying a yellow-white color, indicative of an older stellar population. The galaxy exhibits a relatively thin disc oriented nearly edge-on to our line of sight. This disc shows a mottled appearance with hints of blue color, suggesting the presence of regions of active star formation. There appears to be some minor dust lane obscuration visible along the equatorial plane of the galaxy. There are no obvious signs of major mergers or tidal disturbances. The color gradient across the galaxy suggests a radial population gradient, with younger stars concentrated within the disc and older stars dominating the bulge.
