The galaxy presents a generally smooth and somewhat elongated morphology. There is evidence of a bulge, appearing as a concentrated area of yellowish light. The galaxy exhibits a disk-like structure around this central bulge, indicated by a more diffuse, bluish light. There are possible subtle indications of some spiral arm structure within this disk, though they are not clearly defined. Overall, the galaxy does not appear to be undergoing any major interactions or disturbances; its overall shape seems relatively undisturbed. Its color suggests some on-going star formation within the disk, contributing to the bluer light, although the yellower hue of the central bulge likely indicates an older stellar population there. The galaxy's morphology would place it somewhere between a spiral and a lenticular galaxy, leaning somewhat towards the smoother and more bulge-dominated lenticular classification.
