The galaxy presents a predominantly smooth morphology, with a roughly elliptical shape. The light distribution appears concentrated towards the center, with a gradual decline in intensity outward. The core region exhibits a yellowish hue, suggesting an older stellar population. A bluer, more diffuse area is visible at the galaxy's edge suggesting some possible star formation. There is no strong indication of spiral arm structure or a prominent dust lane. The galaxy's structure appears largely undisturbed; however, the hint of blue may be suggestive of potential minor interactions or a past disturbance of some kind.
