The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light profile. The color gradients suggest an older stellar population, with the central region appearing more yellow. The galaxy exhibits a high degree of rotational symmetry, with a minor axis ratio of approximately 0.49. There is no clear evidence of spiral arm structure or dust lanes. The surface brightness distribution is consistent with a high Sersic index, indicative of a bulge-dominated system. The size of the galaxy suggests that it is approximately 2 Kpc in radius. The galaxy shows a notable red shift, at approximately z = 0.084, and exhibits a color index of approximately 2.3 between the u and r bands. This is consistent with a very old stellar population.
