The galaxy appears to be an elliptical galaxy with a smooth, diffuse light distribution. The object has a concentrated central bulge that appears yellowish-white, gradually fading into an extended, less luminous halo. The halo exhibits a subtle color gradient, shifting towards a greenish hue at its periphery. There are no visible spiral arms or distinct dust lanes present. The overall morphology suggests an older stellar population with limited ongoing star formation, consistent with its smooth appearance and lack of blue coloration. The roundness and lack of strong tidal features suggest it is not currently undergoing any major mergers, although there might be some minor perturbations present.
