The galaxy presents an overall elliptical morphology, though slightly elongated, trending toward a cigar shape. Its central region exhibits a concentrated, bright, yellowish-white glow, likely indicative of an older stellar population. Moving outwards, the color shifts to a slightly bluer hue, suggesting more recent star formation occurring within the galaxy's extended disk. There's a slight hint of spiral structure, or at least some structural feature, that is not well-defined. There's also no major disturbances or mergers visible.
