The galaxy presents a mostly smooth morphology, with a centrally concentrated light profile. Its overall shape appears to be elliptical, with a moderate ellipticity, appearing as a flattened spheroid rather than a perfect circle. There's a hint of a disk component that could be present, but it's not distinctly visible from this angle and resolution. The galaxy's core is significantly brighter and yellower than its outer regions, suggesting a concentration of older stellar populations and dust. A blue hue emanates away from the core, perhaps indicating the presence of younger, hotter stars. There is little evidence of spiral arms, active star formation regions, or major tidal disturbances. The galaxy appears relatively isolated and undisturbed.
