The galaxy appears as a centrally concentrated, luminous object. The light is brightest in the core, diminishing gradually outwards. The overall shape is elliptical, showing high degree of central concentration and smoothness with no obvious spiral arm structure or significant dust lanes visible in the image. There is a subtle color gradient from a brighter, slightly yellowish-white core to a bluer, less intense outer region, potentially indicating ongoing star formation. The galaxy exhibits a regular, non-disturbed morphology and is considered isolated, showing no signs of merging or tidal interactions. Overall, this galaxy can be classified as an elliptical galaxy with possible star formation in the outer regions.
