The galaxy appears as a moderately bright, elliptical or lenticular object with a smooth, featureless morphology. It exhibits a concentrated central bulge that emits primarily yellow light, suggesting an older stellar population. The galaxy is surrounded by a fainter, more diffuse halo that extends approximately four times the radius of the core. There's no evidence of spiral arms, bar structures, or ongoing star formation. The overall color index indicates that this is likely a red-sequence galaxy with little current star formation activity and an estimated diameter between 15-20 thousand light years. There is no indication of active galactic nuclei activity based on the light in this image, and no major interactions or disturbances are readily apparent in its structure, although there is a slight possible visual disturbance on the lower right.
