The galaxy appears as a centrally concentrated, relatively smooth object with an elliptical morphology. The central region is noticeably brighter and exhibits a yellowish hue, suggesting an older stellar population. Moving outward, the galaxy appears to fade gradually into a more diffuse, greenish halo. There is no clear evidence of spiral arm structures or significant dust lanes. The overall structure indicates a mature system, likely dominated by evolved stars, with possibly low levels of ongoing star formation activity within the central regions. The object appears relatively isolated with no obvious signs of tidal interactions or major disturbances from nearby galaxies.
