The galaxy appears as an elongated, disk-like structure. The primary axis is oriented horizontally in the image. A bright central bulge is evident, concentrated and emitting significant light. The disk component is less defined, showing hints of spiral arm structures, although these are faint and possibly disturbed. The color profile suggests a mixture of stellar populations, with bluer hues potentially indicating regions of active star formation within the disk. There are hints of tidal disturbances, indicating a possible interaction with another galaxy, although no companion is obviously visible. Overall, the galaxy presents a complex morphology, requiring further investigation to determine its precise classification and evolutionary state. 
