The galaxy appears as a single, concentrated luminous object, exhibiting a smooth, elliptical morphology. There is no apparent disk structure or spiral arm features visible. The light distribution is centrally concentrated, decreasing gradually outwards. The overall shape suggests a high degree of sphericity, with minimal deviation from a circular profile. There is no indication of any ongoing major merger activity or significant tidal disturbances. The central region displays a yellowish hue, possibly indicating an older stellar population with lower star formation rates.
