The galaxy appears to be elliptical in morphology. It exhibits a smooth, centrally concentrated light profile with a slightly elongated shape. The core is a bright yellowish color, suggesting an older stellar population and relatively low levels of recent star formation. The outer regions of the galaxy fade in intensity and show a subtle color gradient, shifting towards redder hues. This may indicate a decrease in metallicity or age of the stellar populations in the outer regions. There is no visual evidence of spiral arms, a distinct disk structure, or any major ongoing merger events. Minor asymmetry may be present, possibly due to minor interactions. Overall, the galaxy presents as a relatively undisturbed, evolved system.
