The galaxy appears to be a spiral or lenticular type galaxy, exhibiting a generally smooth and rounded morphology. It has a bright central bulge that graduates outward into a fainter disk. The colour of the bulge is consistent with an older stellar population. There are features within the disk, indicating some substructure and potential spiral arm segments. There is evidence of ongoing star formation within the galaxy, as indicated by the presence of blue regions. There may be some form of interaction or disturbance, as there are hints of irregularities in the outer regions. However, no major merger is in progress.
