The galaxy presents as a spiral type, with a notable disk structure. A central bulge is visible, exhibiting a more concentrated, yellowish luminosity. Two main spiral arms appear, each with tightly wound arms that extend outwards from the bulge in a symmetrical manner. There is an absence of a clear bar structure.

The disk shows some degree of inclination relative to our line of sight; The dust lanes can be seen in the spiral arms, obscuring some of the light from stars behind them. The overall color gradient suggests a relatively mature stellar population, particularly within the bulge. There is a subtle hint of bluer regions in the spiral arms which may indicate areas of recent star formation. No significant merger activity or tidal disturbances are immediately evident.
