This galaxy appears to be a relatively smooth, elliptical-like structure, with a centrally concentrated light profile. There is no apparent spiral arm structure or significant dust lanes visible. The galaxy's color exhibits a gradient, transitioning from a somewhat bluer hue in the outer regions to a redder and potentially older stellar population concentrated towards the galactic core. Its morphology suggests it is likely a massive galaxy with limited ongoing star formation. Overall, the galaxy presents a largely undisturbed appearance, indicating it is not currently undergoing a major merger or significant tidal interaction with other galaxies, though there may be minor disturbances.
