The galaxy presents as a disk-shaped structure, elongated along its major axis. It displays a central bulge, exhibiting a yellowish-orange hue, suggestive of an older stellar population. A flattened disk surrounds the bulge. The disk appears to have a greenish tint, indicating the presence of ionized gas and potentially ongoing star formation. Hints of reddish regions within the disk may indicate areas of dust obscuration or the presence of older, redder stars. The overall structure gives the impression of a spiral galaxy viewed at a high inclination angle. There may be some minor disturbances that could imply a merger but nothing seems to be significantly disrupting the morphology. The galaxy appears moderately luminous.
