The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its light profile suggests a centrally dominant elliptical or lenticular type, with no readily discernible spiral arm structures or significant dust lanes. The galaxy exhibits a color gradient, appearing somewhat bluer toward the core and redder towards the outer edges. There is no evidence of a close companion or ongoing major merger activity, although minor disturbances can't be ruled out. The overall shape is close to round, showing no major elongation or bar-like structure. Given the color, the galaxy is likely to be of relatively mature stellar population, although there are hints of some ongoing, albeit low, levels of star formation.
