The galaxy appears to be an elliptical galaxy, displaying a largely smooth morphology. There is some evidence of faint disk-like structure, but overall it is dominated by a spheroidal shape. The central region exhibits a bright, concentrated core, which fades gradually outwards. Color analysis indicates a redder hue, suggesting an older stellar population with lower rates of star formation. The galaxy appears relatively undisturbed, with no signs of ongoing major mergers or tidal interactions. There may be a very minor asymmetry or disturbance present.
