The galaxy exhibits a generally elliptical morphology, though some irregularities are apparent. A bright central bulge is evident, potentially indicative of a supermassive black hole and significant stellar density. Faint, diffuse spiral arm structures appear to emanate from the central bulge; however, these arms are not well-defined and exhibit signs of disruption. The overall color of the galaxy suggests a mix of stellar populations, with a slightly bluer hue in the outer regions possibly indicating ongoing star formation, and yellower colors within the central bulge. There is evidence of possible minor tidal disturbances or interactions with other galaxies, indicated by the slightly asymmetrical shape and faint extensions or streams of light extending outward from the main galactic body. These tidal features need more observation for confirmation. The galaxy does not obviously demonstrate features that are typical of a highly disturbed merging system.
