The galaxy presents a largely smooth morphology, with a dominant central bulge region. It is neither distinctly elliptical nor spiral in appearance, possessing features intermediate between the two. The central bulge exhibits a yellowish hue, indicative of an older stellar population. There is a faint disk present, displaying hints of bluish regions, potentially representing areas of ongoing star formation. Some faint irregularities are present within the disk, which may be the result of minor gravitational interactions. No signs of a major merger are seen. The galaxy is of considerable size and possesses a fairly high estimated mass. Its star formation rate is low for its mass. 
