The galaxy presents a largely smooth, elliptical morphology. The light profile appears centrally concentrated, exhibiting a gradual decline in intensity with increasing radius. The core region displays a yellowish hue, potentially indicative of an older stellar population. Fainter, bluer light is observed in the outer regions which may indicate ongoing or recent star formation but the data suggests a low rate of star formation. Overall, the galaxy shows little evidence of spiral arms, bars, or other significant morphological features, supporting its classification as an elliptical galaxy. There is no evidence of tidal disturbances or any indication of ongoing merging activity.
