The galaxy presents a smooth, elliptical morphology with a relatively high degree of central concentration. The light distribution appears centrally bright, with a rapid falloff in intensity moving outwards, suggesting a dominant spheroidal component. The galaxy exhibits a subtle elongation, but lacks any apparent spiral arm structure or prominent dust lanes. The color profile indicates a redder hue, with light concentrated towards the longer wavelengths suggesting an older stellar population. Overall, the galaxy appears as a relatively undisturbed, evolved system.
