The galaxy appears to be a spiral type, exhibiting a disk-like structure. The central bulge is prominent and moderately sized. Faint spiral arms are suggested, though not sharply defined. The galaxy appears largely undisturbed, with no obvious signs of major mergers or significant tidal interactions. The color distribution implies ongoing star formation, as indicated by a bluish hue in the less defined spiral arms, contrasting with the yellower central bulge which is likely populated by older stars. The overall morphology suggests that the galaxy is viewed at a relatively small inclination angle, showing a face-on orientation.
