The galaxy presents a generally smooth morphology with a slight elongation. It is characterized by two distinct, centrally concentrated regions of higher luminosity separated by a faint bridge. The primary, lower region appears more compact and uniformly bright with a bluish hue. The secondary region is larger and appears to be more diffuse, displaying a slightly less intense, but still evident, blue color. The galaxy exhibits an overall intermediate color profile suggesting ongoing star formation activity. There is no obvious indication of significant spiral arm structure or major disturbances due to mergers, although a possible minor interaction cannot be entirely ruled out given the observed morphology.
