The galaxy presents as a spiral type, with a dominant disk structure. The spiral arms appear tightly wound, exhibiting a flocculent morphology. There is no clear bar structure. The central bulge is moderate in size, but not dominant. The color profile suggests a mixture of stellar populations, with a yellower central region indicative of older stars and dust extinction. There are faint hints of blue indicating star forming regions within the spiral arms. There is no evidence of major interactions or mergers, though some minor disturbances or irregularities might be present in the disk structure.
