This galaxy appears to be part of a system possibly undergoing a merger or strong interaction. There are two distinct components visible: a brighter, slightly more compact, elliptical-like core and a more diffuse, less defined mass to the left. A faint bridge of material appears to connect these two components, suggesting a tidal interaction.

The brighter core shows a smooth light distribution, consistent with an older stellar population. The left component shows a patchy distribution suggesting the presence of younger stars or dust lanes within the galaxy. There may be some signs of tidal tails extending away from the main body of the galaxy system. Overall, the system presents itself as a intermediate mass galaxy with hints of ongoing star formation.
