The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. There is no discernible spiral structure or distinct disk component visible in this image, suggesting an elliptical or lenticular classification. The color profile indicates a predominantly older stellar population, with a yellowish hue dominating the galaxy's central region. The object is approximately round in appearance, with a slight deviation towards an elliptical shape. There is no visual evidence of ongoing major mergers or significant tidal disturbances.
