The galaxy presents a disc-like morphology, viewed at a slight angle relative to edge-on. Spiral arm structures are discernible, exhibiting a generally grand-design appearance, with two dominant arms readily apparent. The arms themselves show a medium winding pattern, neither tightly wound nor loosely extended. A central bulge is clearly visible, exhibiting a moderate size relative to the overall galaxy. Within the disc, there appear to be regions of active star formation, judging from the subtle variations in color and texture. No significant distortions or signs of major mergers are evident; however, the overall appearance suggests some form of minor tidal disturbance is possible. The presence of a weak bar-like structure is suggested by the isophotal twisting evident in the central region. The galaxy's light appears to be dominated by colors associated with older stellar populations, though some pockets of bluer light, indicative of more recent star formation, can be observed within the spiral arms.
