The galaxy appears to be an elliptical galaxy, with a smooth, relatively featureless morphology. It exhibits an elongated shape, potentially classified as cigar-shaped. There are no readily apparent spiral arms or a distinct disk component. The light is concentrated towards the center, suggesting a high degree of central mass concentration. The color profile is predominantly redder, indicating an older stellar population with relatively low levels of ongoing star formation. There is no visual evidence of any major ongoing mergers or significant tidal disturbances, and the overall structure appears relaxed and stable.
