The galaxy exhibits a morphology consistent with a lenticular or early-type spiral galaxy, viewed at an oblique angle. The central region displays a bright, relatively smooth bulge, yellow in color, suggestive of an older stellar population. A disk component surrounds the bulge, appearing more flattened. The disk shows hints of structure, possibly faint spiral arms, but they are not well-defined. The galaxy appears relatively isolated, with no obvious signs of strong tidal interactions or ongoing mergers. The galaxy is slightly tilted with respect to our line of sight, allowing a partial view of the disk structure. The overall color gradient suggests a radial distribution of stellar populations, with older, redder stars concentrated in the bulge and potentially younger, bluer stars residing in the disk. No prominent dust lanes are apparent. The overall appearance is consistent with a galaxy that has largely exhausted its gas supply, with a declining rate of star formation.
