The galaxy presents a somewhat irregular, elongated shape, possibly indicative of a late-type spiral or dwarf irregular galaxy. It exhibits a bluish hue, strongest in the central region, suggesting the presence of relatively young, hot stars and ongoing star formation. The light profile appears somewhat smooth, although there are hints of faint, extended structures or possibly faint spiral arm segments at either end of the main body of the galaxy. Dust lanes are not readily apparent. There's a subtle clumpy nature to the galactic light, potentially indicating star-forming regions within. The galaxy does not show obvious signs of a recent major merger, but a low-level disturbance or minor interaction cannot be ruled out based on morphology alone. The object appears relatively faint. 
