This galaxy exhibits a notable disk structure with a clear, though not sharply defined, spiral arm morphology. The arms appear somewhat flocculent, suggesting ongoing or recent star formation activity distributed along their lengths. The central bulge is prominent, exhibiting a moderate size relative to the overall galaxy disk. The bulge displays a yellowish hue, possibly indicating an older stellar population with reduced star formation. There's some evidence of a bar-like structure within the central region, elongating the bulge. The disk appears to be slightly inclined relative to our line of sight, contributing to its ellipsoidal appearance. There are no readily apparent signs of major mergers or significant tidal disturbances within the galaxy's morphology; however, some faint irregularities in the outer disk might suggest minor interactions. The overall color profile indicates a relatively evolved system.