The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an overall elliptical morphology with a slight deviation from perfect roundness. The light distribution appears relatively uniform throughout the galaxy, indicating a lack of prominent spiral arm structures or distinct star-forming regions. There is a subtle elongation in its shape, suggesting a possible transition between elliptical and lenticular morphology. Minimal disturbances or interactions are visible, indicating the galaxy appears relatively isolated and undisturbed. The galaxy exhibits a moderate luminosity. Color gradients are subtle but appear to be redder in the central region, with bluer hues towards the outer edges, suggesting the presence of older stellar populations in the core. The galaxy does not show any obvious signs of a recent major merger or significant tidal interaction. The object's structure suggests a system that has largely completed its star formation and is dominated by an older stellar population.
