The galaxy presents a generally smooth, elliptical morphology. It appears to be relatively massive and exhibits a moderate redshift, suggesting it is at a significant cosmological distance. The central region is brighter and more concentrated, fading gradually towards the outer edges. The color profile is redder overall, implying an older stellar population with less ongoing star formation. There is a slight suggestion of a disk, but not prominent. No major disturbances or strong tidal features are apparent, though some minor irregularities may be present, possibly indicating a past minor merger event.
