The galaxy exhibits a generally elliptical morphology with a high degree of central concentration. The light is predominantly smooth, with no obvious spiral arm structures or dust lanes visible in this observation. There appears to be some asymmetry to the outer halo. The light profile suggests a relatively old stellar population, with a redder hue dominating the core region, transitioning to slightly bluer tones in the extended halo. The shape is not perfectly circular, indicating some degree of flattening. There is no evidence of a strong tidal interaction or ongoing merger activity, although there might be a faint disturbance. Overall, the galaxy appears to be a relatively quiescent system.
