The galaxy appears to be a relatively compact elliptical or lenticular type. It exhibits a smooth, diffuse light profile, suggesting an older stellar population. The central bulge is prominent and displays a yellowish-orange hue, indicative of evolved stars. No distinct spiral arm structure or dust lanes are discernible, further supporting a classification toward the elliptical end of the Hubble sequence. The galaxy appears mostly undisturbed, with no signs of a major ongoing merger. There is a slight elongation observed, deviating from a perfectly circular morphology.
