The observed galaxy presents a disk-like morphology, viewed at a significant inclination relative to our line of sight. The central bulge region exhibits a yellowish-orange hue, potentially indicative of an older stellar population and/or dust obscuration. Moving outward from the bulge toward the edges of the galaxy, a faint blueish tint can be observed, suggesting the presence of younger, hotter stars perhaps within spiral arm structures. The overall structure of the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. However, there is a very slight asymmetry in the outer regions, which might point to a minor interaction. There appears to be an absence of distinct, well-defined spiral arm features. Overall, it appears to be a spiral galaxy with a fairly high mass, and low ongoing star formation. 
