This galaxy presents as a relatively smooth, disk-like structure with a concentrated central bulge. The overall shape appears somewhat elongated, but not strongly barred or cigar-shaped. The galaxy exhibits a radial color gradient, with a bluer hue towards the outer regions of the disk and a redder, more concentrated color within the bulge, indicative of potentially older stellar populations in the center. The disk shows some hint of spiral arm structure but the arms appear tightly wound and not very well defined. There are no obvious signs of major mergers or significant tidal disturbances, although a minor asymmetry is suggested by a slight warp in the disk on one side. Based on the observed light profile, the galaxy is likely dominated by an intermediate-mass stellar population and exhibits a moderate rate of star formation.
