The galaxy presents an elongated, somewhat cigar-shaped morphology. Its light is dominated by a smooth, centralized bulge that appears yellowish-white, potentially indicating an older stellar population. A faint disk component is suggested by the slight extension of the galaxy along its major axis, although distinct spiral arms are not visible. The disk seems relatively smooth and featureless. There may be a small area of active star formation on the edge of the galaxy, or a foreground element that has appeared on this image, with redder emission. Overall, the galaxy exhibits a relatively undisturbed structure. The faintness of the disk compared to the bulge suggests a system where bulge formation and evolution may have been more dominant than disk activity, or potentially that star formation in the disk has diminished over time.
