The galaxy presents as a luminous object, exhibiting a concentrated central region. The overall form appears smooth and somewhat elliptical, with a hint of disk-like structure, though it is difficult to discern distinct spiral arms. A faint plume or tidal tail extending from the main body suggests a possible past interaction or merger event, however, it is likely not currently undergoing a major merging event or disturbance. The color profile indicates moderate star formation within the galaxy.
