The galaxy exhibits a generally elliptical morphology. A central bulge region, characterized by a high surface brightness, displays a pronounced luminosity. The surrounding disk shows evidence of spiral arm structures, albeit somewhat irregular and not sharply defined. There is a color gradient observed, transitioning from a bluer hue in the central regions outward to greener color. The edges of the galaxy appear somewhat irregular with an estimated radius of approximately 4 arcseconds. The galaxy appears to be relatively isolated, showing no distinct signs of a major merger event, although some minor disturbances or interactions cannot be ruled out from this image alone. The overall structure suggests a transition type, lying between a pure elliptical and a well-defined spiral galaxy.
