This galaxy appears to be a spiral galaxy viewed at an oblique angle. The galaxy exhibits a clear central bulge, somewhat elongated, suggesting it is not perfectly spherical. Surrounding the bulge is a disk component, discernable by its bluer color, especially on one side, likely due to the presence of younger, hotter stars. The disk shows evidence of some structure, possibly spiral arms, although the image resolution limits a detailed analysis. There's also the possibility of a slight warp or tidal disturbance present on one side of the disk, though this could be an artifact of the viewing angle. It appears moderately massive and exhibits a relatively low rate of star formation. There is a clear absence of any major merging events. 
