The galaxy exhibits a disk-like morphology, though the image quality makes precise classification challenging. It appears largely smooth with a bright, concentrated central bulge. The central region displays a bluish-white hue, suggestive of younger stellar populations or active galactic nucleus activity. A less prominent ring of greenish light surrounds the center, indicating the presence of ionized gas or a region of ongoing star formation. Hints of redder emission are observed within the disk, possibly indicating older stellar populations or dust. The overall shape is somewhat disturbed or irregular, suggesting a possible interaction or merger event in its past or present. Faint tidal features extending from the main body of the galaxy cannot be ruled out based on this image alone. The observed colors suggest that the galaxy contains a mix of stellar populations.
