The galaxy presents with a somewhat elliptical morphology, appearing mostly smooth and concentrated towards the center. There is some evidence of a disk-like structure, though it appears disturbed and indistinct. The central region exhibits a bright, concentrated luminosity, suggesting a substantial core. The overall color profile indicates a mix of stellar populations, with a yellowish-white central bulge and hints of bluer regions in the surrounding disk, possibly indicative of ongoing star formation. Irregular features are present suggesting there may be minor disturbances within the galaxy structure, indicating a possibility of recent or ongoing interaction or mergers.
