The galaxy appears to be a spiral galaxy, viewed at a moderate angle, possibly slightly inclined. The central bulge is prominent and exhibits a yellowish-orange color, which may indicate an older stellar population. The spiral arms are not sharply defined, displaying a somewhat flocculent structure. There is a slight bluish tint to the arms, which could indicate the presence of younger, hotter stars and ongoing star formation. The overall appearance suggests a galaxy of intermediate mass with a moderate star formation rate. There are no strong indications of a recent major merger, although some minor disturbances can't be ruled out due to the somewhat irregular appearance of the spiral arms.
