The galaxy presents an elliptical morphology, appearing largely smooth and concentrated. A bright central bulge dominates the galaxy's structure, exhibiting a yellowish hue. The galaxy is slightly elongated, displaying a deviation from a perfectly circular shape. There is a gradual decrease in luminosity from the core outwards. The outskirts show a subtle color gradient, transitioning to slightly bluer tones. No distinct spiral arm structures or significant dust lanes are apparent within the visible spectrum. There are no clear signs of major mergers or tidal disturbances, though minor asymmetries might be present upon closer inspection. Overall, the galaxy appears to be a relatively quiescent system, likely dominated by an older stellar population and exhibiting low ongoing star formation activity.
