The galaxy presents as a relatively smooth, disk-shaped structure. It displays a prominent central bulge that appears nearly spherical and exhibits a yellowish hue, suggesting an older stellar population concentrated in this region. The disk component of the galaxy shows a slight elongation, indicating it is viewed at a moderate inclination. The color gradient transitioning from the central bulge to the outer regions hints at potential differences in stellar populations and composition. Faint hints of spiral arm structure are tentatively discernible within the disk, but these features are not strongly defined. The overall appearance points toward a galaxy with a relatively quiescent star formation rate, with a substantial portion of its stellar mass already formed. There are minor indications of tidal disturbance, but the overall morphology suggests the galaxy is relatively isolated and not currently undergoing a major merger event. The structure of this galaxy points toward an intermediate morphological type, possessing traits of both elliptical and spiral galaxies.
