The galaxy presents as a largely featureless, elliptical-like structure, with a smooth and concentrated central region emitting strongly in the g-band. The overall shape appears nearly circular. Little evidence of spiral arms, bars, or other distinct features is apparent. The redder, outer regions fade gradually into the background, suggesting a smooth stellar density profile. The galaxy exhibits a redshift of approximately 0.27, indicating a significant distance. There appears to be low ongoing star formation within the galaxy. There is no visual evidence of any major merging activity or tidal disturbances.
