The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless light distribution. The central region displays a concentrated brightness, suggesting a significant stellar population density. The color profile indicates a predominantly older stellar population, with a yellowish hue that gradually fades towards the outer regions of the galaxy. There is a subtle departure from perfect circularity, appearing slightly elongated. A lack of distinct spiral arms or dust lanes is evident. No significant tidal features or signs of recent major mergers are apparent; however, a hint of minor asymmetry could be present.
