This galaxy exhibits a morphology that is neither purely elliptical nor spiral, presenting instead a lenticular or possibly a disturbed spiral structure. The primary body of the galaxy is characterized by a smooth, centrally concentrated bulge, exhibiting a yellowish-white hue indicative of an older stellar population. There is also a fainter region extending out from the body. An interesting feature is the apparent distortion on one side, including a reddish area that may be a region of intense star formation. The overall luminosity suggests a relatively massive system with a rate of star formation is slow compared to its mass. Evidence indicates the possibility of some type of galactic interaction or disturbance influencing the morphology.
