The galaxy presents a largely smooth and centrally concentrated morphology. There is an evident radial brightness gradient, with the highest luminosity concentrated in the central region of the galaxy, decreasing gradually outwards. The galaxy appears to be largely spheroidal in shape, exhibiting only a small degree of ellipticity and a low probability of ongoing merger activity or major disturbances. Based on the color profile and observed characteristics, star formation activity appears to be low within this galaxy. The galaxy demonstrates a redder color profile, especially in the central regions.
