The galaxy presents a largely smooth, elliptical morphology. Its light profile appears highly concentrated toward the center, with a bright, yellowish core that suggests an older stellar population. The overall color is relatively uniform, with subtle hints of bluer hues in the outer regions, possibly indicating some level of ongoing, albeit subdued, star formation. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy appears isolated, showing no significant signs of tidal interactions or recent mergers, although a very minor asymmetry is present. Its shape is very close to perfectly round.
