The galaxy presents as a relatively smooth, centrally concentrated object. There is an elliptical shape with an aspect ratio that appears close to round. A bulge is visible as a brighter central region. This bulge is surrounded by what appears to be a fainter, diffuse disk. There is little evidence of spiral arms or dust lanes within the disk, suggesting it may be composed primarily of older stars. I do not observe any indications of major mergers or significant tidal disturbances in this image. The galaxy exhibits a redder color, potentially indicating a higher proportion of evolved stars and lower ongoing star formation within the galaxy. 
