The galaxy presents a largely smooth morphology, with a dominant, centrally concentrated light profile. The overall shape appears close to circular, exhibiting minimal ellipticity. There is a slight color gradient, with a yellowish-white core that may indicate a relatively older stellar population. No distinct spiral arms or bar structures are visible, suggesting it may be either an elliptical or a lenticular galaxy, or a face-on spiral galaxy.

There appears to be a minor asymmetry or irregularity within the diffuse outer regions of the galaxy's light distribution, but this may be due to noise or a minor interaction with another galaxy. There is no evidence for a major ongoing merger event. The blue light visible in the periphery may indicate a small amount of star formation taking place. Overall, the galaxy's morphology appears to be relatively undisturbed.
