The galaxy presents as a smooth, centrally concentrated object, likely an elliptical galaxy. It appears to be elongated, exhibiting a cigar-like shape rather than a perfect sphere. There is a noticeable color gradient, transitioning from a yellowish hue in the core to bluer tinges in the outer regions. This may indicate a younger stellar population in the outer regions compared to the older, redder stars concentrated towards the center. There is no visual evidence of a prominent disk or spiral structure. Faint hints of a potential tidal feature or minor disturbance might be present at the edges, but this is not definitive. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger.
