The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution. There's a central concentration of light, indicating a possible bulge. Faint extensions or tidal features, potentially signifying past or ongoing interactions, are tentatively observed. Color gradients suggest variations in stellar populations across the galaxy. The redder hues may indicate older stellar populations, while the presence of bluer tones, particularly toward the center, could indicate recent or ongoing star formation. Based on its smoothness, it is likely an elliptical galaxy. There appear to be remnants of a merger in this galaxy, which may be causing more star formation than would normally be observed in an elliptical galaxy.
