The galaxy presents a largely elliptical morphology with a smooth, diffuse light distribution. The core is centrally concentrated and exhibits a bright, relatively uniform luminosity across its visible extent. The galaxy's light profile gradually fades into the background, exhibiting a near-circular shape. No distinct spiral arms or prominent dust lanes are discernible within the image. Overall, the galaxy appears to be a relatively evolved system with a predominantly older stellar population. There appears to be minimal evidence of recent major merger events or significant star formation activity within the visible portion of the galaxy.
