The galaxy presents as a primarily smooth and centrally concentrated object, with a slight elongation, appearing as mostly "in-between" and not fully round. The central region exhibits a bright, concentrated luminosity, potentially indicative of an active galactic nucleus or a dense stellar population. The galaxy displays a yellowish-greenish hue, which may reflect an older stellar population and moderate star formation, suggesting a system transitioning from blue starburst activity to redder, more quiescent phases. There are no readily discernible spiral arms or significant dust lanes visible in this image; the galaxy maintains a relatively uniform and featureless appearance, possibly an elliptical galaxy. There is no visible evidence of major mergers or tidal disturbances, although some very subtle asymmetries might indicate a minor interaction in the recent past.
