The galaxy exhibits a generally smooth morphology, appearing largely featureless. It displays a highly elliptical shape, elongated significantly along one axis. The color profile shows a distinct radial gradient, transitioning from a bluer hue in the central regions to redder tones towards the outer edges. This color gradient suggests a potential difference in stellar populations, with younger, hotter stars concentrated in the core and older, cooler stars dominating the periphery. There is no apparent spiral structure or bar-like feature visible, but there is an overall low level of activity with no prominent dust lanes or tidal features.
