The galaxy presents as a relatively smooth, elliptical-like structure with a discernible core. The central region exhibits a pronounced yellowish-orange hue, suggestive of an older stellar population and lower levels of ongoing star formation. The outer regions display a bluish tint, hinting at the presence of younger, hotter stars. There is no apparent spiral arm structure or bar visible, and the overall morphology appears regular, showing only a hint of minor disturbances, suggesting past minor interactions. The galaxy exhibits a slight elongation, leaning more towards an "in-between" shape that is not distinctly round or cigar-shaped.
