The galaxy appears to be a relatively smooth, centrally concentrated object with a noticeable blue hue, suggesting ongoing star formation within its structure. Its morphology is predominantly elliptical or spheroidal, with no apparent spiral arms or a distinct disk. The galaxy exhibits a high degree of roundness.

There is a very minor disturbance in the outer regions of the galaxy.

Based on the colors, we can infer that this is a high mass galaxy, with a low, but present, star formation rate.
