The galaxy presents as a diffuse, somewhat elongated structure, possibly a disk galaxy viewed at a shallow angle. There appears to be a central concentration of light, indicating a possible nucleus or bulge. A noticeable feature is the presence of a bright, compact region offset from the center, appearing intensely blue. This might be indicative of a region of active star formation. The overall color of the galaxy is generally blue, suggesting a population of young, hot stars. There is evidence of some disruption within the galactic disk, possibly from a minor or major merger event. The overall structure appears somewhat disturbed, lacking the distinct spiral arm structure typical of grand design spirals. There is no visible dust lane.
