The galaxy presents as a somewhat elongated, disk-like structure, though dominated by a centrally concentrated bulge. The bulge exhibits a yellowish hue, potentially indicating an older stellar population. Fainter, bluer regions are visible in the outer disk, possibly areas of more recent or ongoing star formation. The overall morphology suggests a disk galaxy seen at a moderately inclined angle. There is no obvious sign of active galactic nuclei or interactions with other galaxies in this image, although there seems to be some possible small dust lanes towards the edge of the bulge, possibly indicating a previous interaction. 
