The galaxy appears as a somewhat diffuse, elliptical object with a noticeable central bulge. The light distribution is not uniform, indicating some internal structure. There seems to be a tidal tail or distorted morphology suggesting a possible interaction or merger event. The object has a dominant yellowish-white core, surrounded by a more extended, fainter halo exhibiting bluish hues. The axial ratio indicates a flattening, and the orientation is at an angle relative to the observer's line of sight. The galaxy exhibits characteristics of a relatively evolved system, with indications of ongoing or past star formation activity. The central region is brighter in the r band than either the g or z bands suggesting the presence of older stellar populations.
