The galaxy presents as a relatively smooth, elliptical morphology. The central bulge is quite prominent and displays a bright yellowish hue, suggesting an older stellar population. Moving outwards from the core, the galaxy fades into a less defined halo, exhibiting a gradual decrease in luminosity. The halo seems to possess a slightly more diffuse and greenish tint. There may be hints of a faint disk structure but it is not prominent. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal disruptions. The shape is somewhat elongated and cigar-shaped.
