The galaxy presents as a relatively smooth, elongated structure. It appears to be an oblate spheroid with a slightly cigar-shaped morphology. The galaxy exhibits a dominant central bulge of moderate luminosity and a diffuse surrounding halo. A hint of a disk can be inferred, but it is not sharply defined. Coloration suggests a complex stellar population. The prominent blue hue concentrated within the central region is indicative of ongoing star formation activity, presumably involving relatively young, massive stars. Redder tones throughout the galaxy hint towards a more evolved population of stars. The apparent lack of defined spiral arms or other detailed features, along with the smooth appearance of the galaxy, suggest a classification leaning towards an elliptical or lenticular type, possibly experiencing a minor disturbance. The galaxy does not appear to be undergoing a major merger, however some sort of interaction cannot be ruled out.
