The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing mostly round with only a slight elongation. The central region displays a brighter, yellowish-white hue, indicating the presence of an older stellar population. Fainter, bluish extensions emanate from the central area, possibly indicating regions of recent or ongoing star formation. The overall structure suggests minimal disturbance or ongoing merger activity, with no clear signs of tidal tails or other major morphological irregularities. The galaxy is observed at a redshift of approximately 0.154, indicating a substantial distance.
