The galaxy presents as a spiral galaxy, moderately inclined relative to our line of sight. The central bulge appears prominent and exhibits a smooth, yellowish-white color, suggesting an older stellar population. Fainter spiral arms extend outward, showing hints of bluer regions indicative of ongoing star formation, particularly on the lower edge of the galaxy. These regions appear patchy and somewhat disorganized. Traces of a weak bar structure may be present across the bulge. No obvious signs of tidal disturbances or major mergers are apparent, though there are slight irregularities in the outer disk indicating a potentially active dynamic.
