The galaxy appears as a centrally concentrated object with a relatively smooth profile. The overall color is yellowish-white, suggesting an older stellar population. There is a slight elongation visible, but the galaxy is mostly circular in appearance. No distinct spiral arms or prominent dust lanes are discernible. Any detailed internal structure appears to be minimal based on this image. There is no evidence of a major ongoing merger, but it's possible minor tidal disturbances might be present, based on slight irregularities in the galaxy's outer regions.
