The galaxy presents as an elliptical morphology, with a high degree of ellipticity. The central region exhibits a concentrated luminosity profile, suggesting a prominent galactic bulge. There is a noticeable color gradient from the center outwards, shifting from a yellowish hue in the core to more reddish tones in the outer regions. This color gradient may be indicative of an aging stellar population and reduced star formation activity in the galaxy's periphery. There is a slight indication of disk structure. There's no clear evidence of spiral arms or significant dust lanes within this system.
