The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The core region exhibits a bright, diffuse glow, suggesting a significant population of older stars. Moving outwards from the center, the light gradually fades, indicating a decrease in stellar density. There's a subtle elongation or 'cigar' shape to the overall structure. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major merger events or tidal disruptions. There's faint hint of a disk structure, but it is not well-defined. The color profile suggests a relatively quiescent star formation rate, with a bias towards redder wavelengths typically associated with an older stellar population.
