The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical or lenticular, exhibiting a high degree of roundness. There is little evidence of spiral arms or significant disk features. The light distribution is centrally dominant, with a gradual decline in intensity towards the outer regions. The galaxy exhibits a yellow-orange color, suggestive of a relatively old stellar population with lower rates of on-going star formation. There is no obvious presence of tidal tails or strong morphological disturbances, indicating the absence of recent major mergers. Faint asymmetric features, such as a very subtle extension or possible tidal stream, are not entirely excluded. 
