The galaxy presents as a flattened, disk-like structure. It is oriented edge-on relative to our line of sight. There is a bright central bulge. Faint, extended emission can be traced along the galactic plane, suggesting the presence of a disk. No distinct spiral arm structure is visible. There may be some evidence of minor tidal disturbances or interactions, as suggested by subtle asymmetries and faint extensions in the immediate vicinity of the galaxy. The galaxy's color appears to be relatively uniform across its visible structure, with a slight concentration towards bluer wavelengths in the central bulge region. The limited z-band data suggest it may be an old system with minimal active star formation, based on the faint features. Overall, this galaxy appears to be a relatively undisturbed, potentially late-type spiral or lenticular galaxy with some morphological peculiarities, possibly due to minor mergers.
