The galaxy presents as a flocculent spiral, exhibiting a disk-like structure. The spiral arms are not well-defined, appearing patchy and fragmented. There is a notable lack of a prominent central bulge; instead, the light is more uniformly distributed across the galaxy. A bar structure is not clearly visible.

The color profile suggests ongoing star formation, particularly within the spiral arms, indicated by the bluish hues. Redder regions are also present, potentially indicating older stellar populations. There is evidence of some disturbance to the galaxy, but there are no signs of a major merger or tidal tail visible. It is a fairly low mass galaxy with evidence of current, low levels of star formation.
