The galaxy presents as a moderately sized, elliptical morphology. It appears largely smooth in texture, with a high degree of central concentration and a diffuse outer halo. The color profile suggests a population of older stars dominating its composition. While it is largely smooth, there seems to be some interaction or disturbance to its morphology. The galaxy has a well defined core that appears round. The image hints at a merging event or tidal interaction contributing to the observed disturbance. The estimated redshift indicates that this object is a considerable distance from our vantage point.
