The galaxy presents as a slightly diffuse and irregular object. The overall structure appears to be dominated by a central bulge that is not particularly pronounced. There is evidence of a possible disk structure, exhibiting faint spiral arms or features. These arms are somewhat ill-defined and patchy. A degree of disruption is observed in the galaxy's morphology, suggesting a possible interaction or disturbance. The color profile suggests ongoing star formation activity, with hints of bluer regions within the galaxy. The galaxy is not particularly bright in this field.
