The galaxy presents as an elliptical or spheroidal system with a smooth, largely featureless morphology. It appears highly symmetrical, exhibiting a round shape with minimal discernible deviation from circularity. The light distribution is concentrated towards the center, suggesting a dominant bulge component. Color gradients within the galaxy are subtle, with a slightly redder hue in the core region, potentially indicative of an older stellar population, and bluer colors further outwards, hinting at younger stars and/or ongoing star formation. There is no evidence of strong tidal features, major mergers, or significant dust lanes. The galaxy exhibits moderate luminosity, characteristic of a massive system. Overall, the galaxy presents a settled state, likely having undergone significant evolutionary processes in the past.
