The galaxy presents as a slightly inclined disk galaxy, exhibiting a generally smooth morphology. A prominent central bulge is visible, which appears to be relatively bright and concentrated. The disk shows some faint spiral arm structure, although it is not sharply defined. The overall color suggests a stellar population that is neither intensely star-forming nor entirely passive. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances. The edges of the disk appear diffuse and slightly blurred. There is no apparent dust lane obscuring the bulge. The general appearance is consistent with an intermediate-type spiral galaxy at a moderate redshift.
