The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light profile, with a gradual decrease in surface brightness towards the outer regions. The galaxy’s core presents a yellowish hue, suggesting an older stellar population. Moving outwards, the color shifts towards a slightly redder tone, further supporting this hypothesis. There is minimal evidence of spiral arm structure or significant dust lanes. The overall morphology suggests a galaxy that has largely completed its major star formation activity. Faint distortions in the outer halo may hint at minor past interactions, but the overall structure is largely undisturbed.
