The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The galaxy appears to be generally round, with minimal discernible disk features or spiral arms. A slight elongation is observed, with the major axis oriented roughly horizontally in the image. The color is predominantly yellow-orange, suggestive of an older stellar population and potentially a lower rate of ongoing star formation within the main body. A subtle extension or possible tidal feature is visible on the left side of the galaxy. This feature has a bluish tint, indicating the presence of younger, hotter stars or perhaps a region of active star formation. The overall appearance suggests a galaxy with a significant stellar mass, displaying characteristics of a system that has largely ceased active star formation, with the exception of the region on the left. Evidence suggests that the galaxy may have recently undergone, or be currently undergoing, a minor merger or tidal interaction.
