The galaxy presents as an elliptical shape with a relatively smooth, albeit somewhat disturbed, morphology. The central region exhibits a bright, concentrated core, suggesting the potential presence of an active galactic nucleus or a dense stellar population. The outer regions of the galaxy display a fainter, more diffuse glow. A faint band or tidal stream on the edges of the galaxy indicates a possible minor merger or gravitational interaction with another galaxy in its past. There are noticeable disruptions in the overall structure. The color profile of the galaxy seems to be relatively uniform, with a slight shift towards blue in the central region, which may point to a population of younger, hotter stars or active star formation in the center.
