The galaxy presents as a spiral type, oriented at an inclined angle relative to the line of sight. A central bulge is evident, exhibiting a moderate size and a yellowish hue suggestive of an older stellar population. Two primary spiral arms are observed, emanating from the central region, demonstrating a fairly tightly wound structure. These arms appear to be the main features and are bluish, indicating a younger population with ongoing star formation. There is no apparent strong bar feature. There are no signs of a major merger or significant tidal disturbance.
