The galaxy presents a generally smooth appearance, with a dominant central bulge exhibiting a yellow-orange hue. This bulge is relatively concentrated and constitutes a significant portion of the galaxy's overall luminosity. There is a faint, diffuse disk component surrounding the central bulge. Within the disk, there appear to be some subtle, irregular features, suggesting possible disturbances or interactions. The disk exhibits a bluer color compared to the bulge. The galaxy is not perfectly round but displays a slightly elongated shape. There is no distinct evidence of a major ongoing merger.
