The galaxy presents a generally smooth appearance, exhibiting a centrally concentrated light profile. The morphology appears to be elliptical with a relatively high degree of roundness, though there is some deviation towards a slightly elongated form. No prominent spiral arms or distinct disk structures are discernible. There is a hint of a possible minor disturbance, with a slight asymmetry present in the outer regions. The color index suggests a relatively old stellar population. No signs of on-going major merger activity are apparent. 
