The galaxy exhibits a mixed morphological profile. Its overall appearance suggests a dominant spheroidal component, evidenced by the largely smooth and concentrated central region. There's an elongated, irregular, disc-like extension, potentially indicating a past interaction or ongoing accretion. The central bulge displays a yellowish hue, suggestive of an older stellar population. Fainter blueish regions are sparsely scattered within the galaxy. There are structural asymmetries and a possible minor disturbance in the morphology, indicating that it could be a merger. The general shape of the galaxy is somewhere in between round and cigar shaped.
