The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light profile. The core exhibits a yellow-white hue, suggesting an older stellar population. The galaxy's outer regions display a slight blue tint, potentially indicating the presence of younger, hotter stars, though this is less pronounced than in spiral galaxies. The shape is generally round but slightly elongated, deviating somewhat from a perfect sphere. There is no apparent spiral structure, bar, or significant dust lane. No major distortions or tidal features are immediately visible, suggesting it is not currently undergoing a major merger, though there might be minor disturbances present. Overall, this galaxy presents a typical morphology for an elliptical galaxy, with evidence of a substantial spheroidal component and an aging stellar population.
