This galaxy appears to be a relatively small, disk-shaped galaxy observed at an oblique angle. The central region exhibits a smooth, concentrated appearance with a bluish hue. The blue color indicates ongoing star formation within this region, likely dominated by younger, hotter stars. The disk component is faintly visible, extending outward from the central bulge, but lacking defined spiral arm structures. There are hints of disturbed morphology suggesting potential past interactions. The overall low surface brightness suggests a lower stellar mass and lower star formation rate. There is a possible minor disturbance present, but it is difficult to confirm. The galaxy does not appear to be undergoing any major merger activity.
