The galaxy appears to be a relatively smooth, elliptical galaxy with a notable central bulge. It exhibits a flattened, disk-like structure although no spiral arms can be definitively identified. The light distribution is concentrated towards the core, gradually fading towards the outer regions. The core exhibits a yellowish-white hue, suggesting an older stellar population, while the outer regions show a slight bluer tint, indicating the presence of younger stars or ongoing star formation, even at a small rate. The galaxy is oriented at an angle relative to our line of sight, with its major axis appearing longer than its minor axis. There is no evidence of any significant ongoing merger activity or tidal disturbances.
