The galaxy presents as a relatively smooth, centrally concentrated light distribution, suggesting an elliptical or lenticular morphology. The main body of the galaxy appears largely featureless. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. A more diffuse, dimmer halo surrounds this core, displaying a gradual fade-out in intensity. There is a slightly redder and more concentrated point of light offset from the core. The galaxy lacks any visible spiral arms or distinct dust lanes. No strong tidal features or morphological disturbances can be identified, implying the absence of recent major merger activity. Overall, the galaxy's light distribution is smooth and regular, with a round to slightly elongated shape.
