The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light profile. It has a generally elliptical shape, with a moderate ellipticity. No spiral arm structures are visible in this image. The color gradient appears fairly uniform across the galaxy, shifting from blue to red light, suggesting intermediate to old stellar populations. There is no evidence of significant dust lanes or prominent star-forming regions. The morphology suggests a system that has largely exhausted its gas supply and star formation has slowed or ceased. There may be a possibility of minor disturbance, which may be due to tidal forces or a possible past merger event.
