The galaxy appears to be composed of two distinct components that are likely interacting. The first component is a relatively smooth, elliptical-like structure, exhibiting a concentrated luminosity profile and a yellowish hue. This suggests a population of older stars with lower rates of star formation.

The second component displays a slightly elongated, less defined structure. It presents a bluer color gradient compared to the first component, hinting at more recent star formation activity within a dusty interstellar medium. There is some evidence of minor tidal disturbance in this component, suggesting a possible gravitational interaction with the other component.

The separation between the two components suggests a close proximity, strengthening the likelihood that the galaxy is in the process of merging or undergoing a significant gravitational interaction. The overall morphology is in between that of a pure elliptical and pure spiral, suggesting this galaxy is in transition.
