The galaxy presents as a relatively compact, spheroidal object. The light distribution appears smooth and concentrated towards the center, suggesting an elliptical morphology. There is some indication of a slight color gradient, shifting from a bluer hue in its core to a redder tone in its outer regions. The galaxy does not exhibit any apparent spiral arms, distinct disk structure, or major disturbances indicative of an ongoing merger. Given the smooth light profile, the galaxy most likely has little to no star formation currently occurring. There is also no indication of strong tidal features or distortions in its shape.
