The galaxy presents a generally smooth, rounded morphology. The light distribution appears fairly uniform, showing no prominent spiral arms or bar structures. The color profile suggests ongoing star formation, indicated by a central bluish hue that graduates to a reddish edge, although it does not appear to be forming a significant number of stars. This suggests that the galaxy may be transitioning away from its peak star-forming phase. There is no evidence of significant tidal disturbances or merging activity, indicating a relatively isolated system.
