The galaxy presents an overall elliptical morphology, appearing somewhat elongated in shape. A central bulge region is discernible, exhibiting a concentrated luminosity. The light distribution appears relatively smooth, suggesting a lack of significant spiral arm structure or prominent dust lanes. There's a subtle color gradient observed, transitioning from a more yellowish hue in the core to a slightly bluer tint in the outer regions, indicative of potential variations in stellar populations or star formation activity across the galactic disk. The galaxy appears to be in a relatively isolated state, with no readily apparent signs of ongoing major mergers or significant tidal disturbances. However, subtle asymmetries or minor disturbances cannot be completely ruled out at this resolution.
