The galaxy presents a generally smooth, elliptical morphology. A central bulge is visible, exhibiting a concentrated luminosity that fades outwards. The color gradient suggests an older stellar population dominating the core region, shifting towards bluer hues in the outer disk. Subtle disturbances are hinted at in the galaxy's structure, possibly indicating past interactions or minor mergers. A relatively low level of ongoing star formation may be present within the galaxy. The roundness of the galaxy is evident, and there is no significant elongation. The majority of the galaxy’s light appears to originate from an older stellar population.
