The galaxy appears to be a disk galaxy, viewed at a significant angle, approaching edge-on. It displays a bright, concentrated central bulge that appears yellowish in color, suggesting an older stellar population is dominant in this region. The disk is visible extending outwards from the bulge. The disk exhibits a bluer hue in comparison to the bulge, which is indicative of ongoing star formation or a younger stellar population, although no prominent star-forming regions or spiral arms are clearly resolved in this image. The overall smoothness and regularity of its structure suggest that it is relatively undisturbed, showing only minor disturbances. The galaxy's shape is moderately elongated.
