The galaxy exhibits a predominantly smooth morphology, with a somewhat elliptical shape. The central region appears as a bright, concentrated bulge of light, suggesting a significant population of older stars. There is subtle evidence of a disk component extending outwards from the core, but it appears disrupted, possibly indicative of a gravitational interaction. The colors suggest a mix of stellar populations, with a redder component at the top possibly related to dust obscuration or older stars and a bluer component in the center representing younger, hotter stars. It is possible this is a merging system, or at least a system with a significant interaction history. 
