The galaxy presents a generally smooth and rounded morphology. It exhibits a bright central concentration of light, which could be indicative of an active galactic nucleus or a dense stellar population. The overall color appears to be a blend of red and green wavelengths, potentially suggesting a mix of older stellar populations and ongoing star formation. There is no obvious disc shape or spiral arm structure. The galaxy displays a relatively undisturbed structure, lacking evidence of any major merging events. The shape is generally round, with slight deviation from a perfect circle. 
