The galaxy presents as a somewhat elongated, elliptical structure. The color distribution appears to have a strong central concentration, with a yellowish hue dominant in the core region, suggesting an older stellar population. The outer regions exhibit a more diffuse, bluish tint indicating the presence of somewhat younger stars. The overall morphology suggests a relatively smooth structure with little to no evidence of spiral arms or significant dust lanes. There might be a slight asymmetry in the outer regions but there is no evidence of recent major merging events.
