The galaxy appears to be a spiral type, possibly an Sa or Sb. It exhibits a central bulge that is relatively prominent and yellowish in color, indicating an older stellar population. The spiral arms are not well-defined, appearing somewhat flocculent. The disk component shows a bluish tint, suggesting the presence of younger, hotter stars and ongoing star formation, though it may be at a relatively low rate. There are some regions with increased redness, potentially due to dust obscuration or redder stellar populations in those areas. The galaxy's overall appearance suggests it is relatively massive and moderately luminous. It doesn't seem to have any obvious signs of a major ongoing merger, but there could be minor disturbances in the outer regions of the disk.
