The galaxy presents a somewhat elliptical morphology, exhibiting a predominantly smooth light distribution. There appears to be a discernible disk structure, although it does not appear perfectly face-on. Subtle disturbances are visible in the disk's outer regions, hinting at possible past minor interactions. The central bulge is apparent and has a yellowish hue, possibly indicating an older stellar population. The overall color suggests it is intermediate in color. There is marginal evidence for recent star formation within the disk.
