The galaxy presents as a disk-shaped system, viewed at a high inclination. A central bulge is not readily apparent; instead, the luminosity appears relatively uniform across the disk. There are some visible disturbances in the galaxy's structure. A faint arm-like feature can be seen extending from the main disk structure. This feature, though subtle, suggests a recent or ongoing interaction with another object.

The color gradient indicates a mix of stellar populations within the disk. The central region exhibits a bluer hue, potentially signifying ongoing star formation. The outer edges appear redder, indicating older stellar populations.

The overall morphology suggests the galaxy is neither purely elliptical nor a grand design spiral, but something in between. 
