The galaxy presents as a relatively smooth, elongated structure, consistent with a disk-like morphology observed edge-on. The light distribution is concentrated toward the center, indicating the presence of a bulge or core region. There is a hint of color variation, with the central region appearing slightly more yellow/red, possibly indicative of an older stellar population or dust obscuration. The outer regions of the disk are less well-defined and appear fainter, potentially due to a lower density of stars and gas at the edges. There does not appear to be any evidence of a major merger or strong tidal interaction, though a subtle disturbance cannot be ruled out. The overall appearance suggests a relatively evolved galaxy with a moderately low star formation rate.
