The galaxy presents as a centrally concentrated, spheroidal structure with a smooth light profile. There is a distinct, bright core which fades gradually into the outer regions of the galaxy, with no clearly visible spiral arms or disk-like features evident. The overall color appears to be trending towards redder hues, indicating an older stellar population. It is relatively round in shape, lacking any significant elongation or asymmetry. The light appears uniform and there are no signs of any on-going merging events or tidal disturbances. Based on these characteristics, the galaxy is likely an elliptical galaxy.
