The galaxy presents a largely smooth morphology, with a dominant spheroidal component. It appears elliptical in shape, showing only a minor deviation from perfect roundness. A central bulge is prominent, exhibiting a concentration of light and a yellowish hue, suggesting an older stellar population. The outer regions are less concentrated and appear slightly bluer, hinting at the presence of younger stars and ongoing, albeit moderate, star formation. There is no obvious evidence of strong tidal distortions or interactions with other galaxies, suggesting it is relatively isolated and undisturbed. No spiral arm structure is discernible.
