The galaxy appears to be an elliptical type, displaying a smooth, centrally concentrated light distribution. There is a noticeable, bright core with a gradual decrease in luminosity towards the outer regions. The overall shape is close to circular, with minimal signs of a disk-like structure or spiral arms. There is no indication of significant dust lanes or patches of active star formation from this imagery, which would be consistent with low star formation rate. The galaxy exhibits a redder color profile with increasing radius, likely indicating an older stellar population dominating the outer regions. No apparent signs of tidal disturbances or ongoing merger events are visible, suggesting it is a relatively isolated and undisturbed system.
