The observed galaxy presents as a moderately sized, disk-shaped structure. Its apparent ellipticity suggests an inclined orientation relative to the observer's line of sight. A central bulge region exhibits a concentrated luminosity, appearing with a bluer hue, likely indicating a higher density of younger, hotter stars. The galactic disk component is less defined, with a somewhat patchy or flocculent appearance. The disk possesses a complex structure with a hint of spiral arm fragments. There is faint evidence of some disturbance. Overall, the galaxy does not seem to be a completely relaxed system, perhaps hinting at past interaction or ongoing minor merging.
