The galaxy appears to be a spiral type, with a predominantly smooth morphology. The central bulge exhibits a bright, concentrated luminosity, suggesting a high stellar density. The disk surrounding the bulge is inclined relative to our line of sight. There is evidence of some structure within the disk, possibly indicative of spiral arms, or perhaps the galaxy has a complex morphology, as the structure looks disturbed, possibly due to a merger. The galaxy exhibits a color gradient, with the central regions appearing more yellow-white and the outer regions showing a bluer hue. This color difference might be due to different stellar populations or dust content within the galaxy. There is only a hint of ongoing star formation.
