The galaxy presents as a centrally concentrated object, exhibiting a smooth and generally elliptical morphology. The light profile shows a radial fall-off from a bright central region, suggesting a substantial bulge component. There is no discernible disk structure, spiral arms, or bar. The overall color is somewhat yellow/orange in appearance, potentially indicating an older stellar population and relatively low star formation rate. We see some suggestion of faint bluer regions in the outskirts of the galaxy, possibly indicating some small amount of ongoing star formation. There does not appear to be evidence of any major mergers or tidal disturbances, although subtle distortions in the outer isophotes could suggest minor gravitational interactions. The galaxy appears relatively isolated and undisturbed.
