The galaxy presents as a single, concentrated object with a centrally dominant, smoothly distributed light profile. There's no apparent spiral arm structure or strong bar feature visible. The galaxy exhibits a somewhat elliptical morphology, with a slight deviation from perfect circularity. The central region is notably brighter and exhibits a yellowish-orange hue, indicative of an older stellar population. Towards the outer regions, the color appears to subtly shift towards redder tones, although this is not very pronounced. There is little to no indication of recent or ongoing major mergers or tidal disturbances in the image, although minor asymmetry cannot be ruled out. Overall, the galaxy appears relatively undisturbed, with a structure consistent with an elliptical or lenticular classification.
