The galaxy presents as a relatively smooth, centrally concentrated object, with a roughly elliptical morphology. There is a noticeable color gradient, transitioning from a bluer hue in the outer regions to a redder, possibly more dusty core. The overall light distribution suggests a galaxy with a dominant spheroidal component, potentially an elliptical or S0 type galaxy. There is a hint of faint structure, possibly a faint disk, but this is difficult to resolve due to the galaxy's distance. There are no obvious signs of strong tidal interactions or a recent merger event, although subtle distortions cannot be ruled out at this resolution. Star formation is likely occurring, though is concentrated in a small central region.
