The galaxy presents as a generally smooth structure with a slight disk-like morphology. The central region exhibits a concentrated brightness, suggestive of a prominent bulge. The overall color appears yellowish-white, indicating a population of older stars. Faint blueish regions on one side hints at regions of star formation. There are hints of minor disturbances within the disk, potentially due to gravitational interactions. The galaxy does not display a clear spiral arm structure, leading to a classification leaning towards lenticular or early-type spiral. It does not seem to be undergoing any major merger events.
