The galaxy presents as a spiral type, exhibiting a generally well-defined disk structure. Prominent spiral arms are visible, displaying a tightly wound morphology. A central bulge is apparent but appears relatively small compared to the overall disk size. The bulge exhibits a yellowish hue, suggesting an older stellar population. The spiral arms show bluer tints, potentially indicative of more recent star formation activity. There is a slight lopsidedness to the galaxy with an indication of a possible merger or tidal interaction as one of the spiral arms looks significantly disrupted or extended. Some asymmetry is present in the light distribution across the disk. There is a distinct cyan coloured object on one side of the galaxy. The is most likely a region of active star formation. There are no signs of a stellar bar. Overall, the galaxy appears to be in a state of active star formation, as suggested by the spiral arm color, and may have undergone, or be undergoing a minor merging event.
