The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology with no discernible spiral arms or distinct features like a bulge or disk. The light distribution is relatively uniform, suggesting an older stellar population. There is a slight color gradient, with the core appearing more yellowish and transitioning to a redder hue in the outer regions. This color shift indicates that the central area may have a higher concentration of older stars than the surrounding regions. There are no obvious signs of recent or ongoing star formation, or any evidence of significant dust lanes. The galaxy appears relatively undisturbed and does not seem to be undergoing any major merger activity.
