The galaxy presents as a luminous, elliptical object with a smooth light distribution. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outwards, the galaxy appears less concentrated and the color shifts subtly towards redder tones. This may indicate a change in stellar population or dust content in the outer regions. Overall, the object appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. There may be very minor asymmetry present but overall it presents a cohesive and relaxed form.
