This galaxy presents as a spiral type, viewed at an angle, with a significant portion of the disk visible. The central bulge appears moderately sized and exhibits a yellowish hue, indicative of an older stellar population.

The spiral arms are well-defined and exhibit a clear winding pattern. The structure suggests the presence of at least two major arms, displaying bright, knotty regions, possibly sites of active star formation. These regions are scattered throughout the arms. 

There appears to be interaction or disruption of the galactic disk and spiral arms with the upper portion of the image displaying a tidal tail like structure. This may be indicative of a prior or ongoing galactic merger event. There doesn't appear to be a strong bar feature.
