The galaxy presents as a relatively smooth, elliptical-like structure. The primary body exhibits a centrally concentrated luminosity profile, indicating a substantial bulge component. The color appears reddish-yellow, suggesting an older stellar population with lower ongoing star formation. There is a secondary, less luminous component located nearby, however, it is difficult to determine from this image alone whether this is part of the galaxy or a separate object. There are no distinct spiral arms or dust lanes visible within the galaxy's disk. The general morphology implies that the galaxy is likely not undergoing any major mergers or significant disturbances. It could be a galaxy near the end of its lifecycle and is no longer forming new stars. 
