The galaxy presents as a spiral type, observed at an angle that is neither face-on nor edge-on. Distinct spiral arms are visible, displaying a somewhat flocculent structure rather than grand design. There is a presence of blue-ish light throughout the arms, which may signify regions of relatively recent or ongoing star formation.

A central bulge appears, with a notable concentration of light. Its color is more yellowish, potentially indicating an older stellar population, but it is difficult to determine the exact bulge-to-disk ratio, or the presence and strength of a bar structure. 

There are irregularities in the morphology, specifically a disturbed appearance. This could be the result of an ongoing or recent merger event with another galaxy, or an internal event that caused a disturbance within the disk. There seems to be an off-center bright portion that could be tidal debris from the suggested disturbance, or an area of intense star formation.
