The galaxy presents a discernible disk structure, exhibiting a distinct spiral morphology. The spiral arms are somewhat flocculent and asymmetrical, suggesting ongoing or recent gravitational interactions.  A central bulge is present, though not overly prominent. The overall color suggests the presence of both younger, bluer stellar populations and older, redder populations. The asymmetry of the spiral arms and presence of distorted structure implies a possible ongoing or recent merger event with a smaller galaxy, indicated by prominent tidal features or disturbances.  There is evidence of active star formation regions within the spiral arms, characterized by a slightly bluer hue compared to the older stellar populations in the bulge. The galaxy appears to be inclined at an angle that is relatively close to edge-on.
