The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be a single, cohesive structure. The light distribution indicates a centrally dominant component, likely a bulge. There are no obvious spiral arms or bar structures evident in this image. The color appears generally uniform across the galaxy. The outskirts of the galaxy gradually fade, suggesting a lack of significant ongoing star formation in those regions. There are no signs of major mergers or tidal disturbances. There are no bright star forming regions or significant dust lanes visible.
