The galaxy presents a morphology consistent with a late-type spiral galaxy, observed nearly edge-on. A prominent disk is visible, displaying a distinct flattening. The central bulge is moderately defined, appearing relatively smooth with a slightly concentrated luminosity. Star formation appears to be primarily located within the disk, which appears somewhat knotty. The disk exhibits a bluer color, particularly towards the outer edges, indicating the presence of younger, hotter stars, which suggest ongoing or recent star formation. No grand design spiral arms are readily discernible, potentially due to the edge-on viewing angle. There may be some minor asymmetry to the galaxy, but there is no indication of significant tidal disruption or merger activity. The overall color suggests it is a moderately massive galaxy with a relatively low star formation rate.
