The galaxy presents a relatively smooth and elongated morphology. The primary structure appears as a spheroid with a moderately elliptical shape, exhibiting a noticeable bulge at its center. The color gradient suggests a concentration of older stellar populations within the central bulge, which is characterized by a reddish hue. Moving outwards from the core, the galactic disk reveals a bluer tint, possibly indicative of younger, hotter stars and regions of active star formation. However, no distinct spiral arms are visible. There is a hint of asymmetry or a minor disturbance in the outer regions of the disk. Overall, the galaxy seems to be undergoing some interactions or recent merger events, though the overall structure is still relatively intact.
