The galaxy presents an elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, with a notable absence of distinct spiral arms or prominent dust lanes. The color gradient suggests an older stellar population, with a reddish hue dominating the central region, possibly indicating a higher concentration of evolved stars. The galaxy appears moderately flattened. There's a subtle hint of bluer light in the outer regions, perhaps indicative of some ongoing, though limited, star formation. The galaxy shows no signs of major mergers or significant tidal disturbances.
