The galaxy presents a complex morphology with a non-uniform light distribution. There is a prominent central bulge, however it is somewhat irregular in shape. Emanating from this central region are faint spiral arms. These arms are difficult to trace and appear somewhat fragmented and disrupted. The colour of the galaxy is overall bluish, suggesting the presence of ongoing star formation, although there are also redder regions. These redder regions may indicate older stellar populations. The galaxy exhibits signs of disturbance or interaction, possibly through a merging event as suggested by a slight asymmetry and some extended features. The nucleus appears relatively bright, but no distinct active galactic nucleus signature is immediately apparent.
