The galaxy presents as a spiral type, exhibiting a disk structure with tightly wound spiral arms that are difficult to discern individually, which could be due to resolution limitations. There appears to be a prominent central bulge with a bright nucleus, indicating a significant concentration of stars. The bulge's size appears moderate relative to the disk. There is a slight indication of a bar-like structure bisecting the bulge, though it is not strongly defined. The overall color of the galaxy suggests a mix of stellar populations, with the central region appearing more yellow-white, potentially indicating older stars. A bluer hue, especially in the areas off the central bulge, may indicate ongoing star formation. There is no readily apparent interaction with another galaxy, nor are there any major morphological disturbances to indicate a recent merger event.
