This galaxy presents as a moderately inclined, disk-dominated system. It appears elongated, with a major axis visually estimated to be several times longer than its minor axis. 

The central region exhibits a relatively smooth, albeit faint, bulge or nucleus. The disk structure is complex, showing evidence of spiral arm segments that are not well-defined but indicated by subtle color variations and clumpy regions. Some of these clumps appear bluer in color, which could signify regions of active star formation.

There is little evidence of a prominent bulge component or a clear, grand design spiral structure. The dust lane may be present, which is typical for an edge-on or high inclination disk galaxy. Overall, the galaxy exhibits some level of disturbance.
