The galaxy presents as a flattened, disk-like structure, viewed at a slight angle. The central bulge is prominent and appears relatively smooth and luminous, exhibiting a yellowish-white hue, suggestive of an older stellar population.

The surrounding disk shows some evidence of structure, though it lacks well-defined spiral arms. The disk appears mottled, with subtle variations in color and brightness, possibly indicative of ongoing, but not vigorous, star formation within. The outer regions of the disk are less distinct and fade gradually into the background, displaying a faint bluish tint. There's no strong evidence of active galactic nuclei activity or major disturbances, suggesting a relatively quiescent state. Overall, it appears to be a relatively large galaxy with a dominant bulge and a moderately sized disk.
