The galaxy presents as an elliptical morphology, exhibiting a smooth and largely featureless profile. The central region is characterized by a high concentration of light, appearing bright and yellowish-white. This suggests an older stellar population dominating the core. Moving outwards from the center, the light gradually diffuses, transitioning to a more subdued bluish hue in the outer regions of the galaxy. The galaxy appears largely undisturbed, lacking any obvious signs of recent merger activity. While not perfectly spherical, the shape is more akin to a flattened spheroid, presenting an intermediate ellipticity. It is a relatively massive galaxy, with a substantial stellar population distributed throughout its volume. There is some evidence of ongoing, though perhaps subdued, star formation activity within the galaxy.
