The galaxy presents as a well-defined disk galaxy, viewed at an intermediate inclination. A central bulge is apparent, appearing bright and somewhat diffuse. The disk exhibits a relatively smooth texture with only hints of spiral arm structure. There is the suggestion of dust lanes obscuring light from the bulge. The galaxy appears relatively isolated. The color profile suggests ongoing star formation, particularly concentrated in the disk region. The overall morphology suggests a galaxy that has largely completed the merging process.
