This galaxy appears to be a relatively smooth, elliptical type. The core exhibits a concentrated yellowish-white light, suggesting an older stellar population. Moving outward, the galaxy appears less concentrated with an apparent disk shape surrounding the core. The galaxy exhibits an overall blue tint to it. There is some indication of disturbances in the galactic structure, most likely a minor disturbance. Overall, it presents as a non-merging system with an intermediate roundness.
