The galaxy presents as a spiral with moderate bulge prominence. There's a hint of spiral arm structure visible, suggestive of a well-defined disk but the spiral arms appear somewhat flocculent. The central bulge exhibits a yellowish hue, likely indicating an older stellar population. The disk itself shows a bluer coloration in some areas outside the central bulge, perhaps indicating areas of more active star formation. The disk seems to have some disturbance and is not perfectly symmetrical. There is an absence of any obvious signs of major merging activity. The orientation is inclined relative to our line of sight, but not completely edge-on.
