The galaxy appears to be a spiral galaxy, displaying prominent spiral arm structures. There is a clear disk component, and the arms are relatively well-defined, exhibiting a slight winding pattern. The bulge of the galaxy is of moderate size, with a yellowish hue, suggestive of an older stellar population. Patches of blueish light are observed in the spiral arms, indicating regions of active star formation. The presence of these blue regions, alongside the overall spiral structure, suggest it is a relatively late-type spiral galaxy. The shape of the galaxy is somewhat disturbed, possibly indicative of a past or ongoing interaction with another galaxy. Further investigation is required to determine the extent and nature of any gravitational disturbances. There is also a slight hint of a bar structure.