The galaxy appears to be a disk galaxy, though the disk is viewed at a moderate inclination. The central bulge is prominent, exhibiting a yellowish hue, possibly indicative of an older stellar population. The disk shows a hint of spiral arm structure with blueish-white regions within the disk, suggesting recent star formation. These regions do not dominate the galaxy's appearance, hinting that star formation is present but not extremely active. The overall shape is elongated, not perfectly round, suggesting it's an intermediate type between a spiral and an elliptical. There is no visually apparent evidence of ongoing major mergers or significant tidal disturbances in the image.
