The galaxy presents as an elliptical or lenticular type, with a generally smooth and concentrated light profile. It appears moderately bright, exhibiting a yellowish-white hue that suggests an older stellar population. The galaxy's core is brighter than its outer regions, showing no clear evidence of spiral arms or significant dust lanes. Overall, its morphology appears undisturbed, showing no signs of major mergers or tidal interactions. The elongated shape indicates the possibility of it being an elliptical galaxy that isn't perfectly spherical. There are no major regions of star formation visible.
