The galaxy presents as a somewhat elongated, cigar-shaped object with a smooth, featureless appearance. The central region exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Progressing outwards, the galaxy fades into a less concentrated and more bluish halo. No distinct spiral arm structures or dust lanes are discernible. The overall morphology suggests a relatively evolved system, possibly an elliptical or lenticular galaxy with ongoing, but perhaps not intense, star formation. There is no indication of any major merger events in the recent past. The galaxy appears relatively undisturbed.
