The galaxy appears as a centrally concentrated, elliptical-like system. The core region exhibits a bright, yellowish hue, indicating a likely population of older stars. A subtle color gradient is observed, transitioning to a bluer periphery. This suggests some on-going star formation activity or a younger stellar population in the outer regions, although it is mostly composed of older stars. The galaxy's overall structure is relatively smooth with no distinct spiral arms or strong features. The system seems isolated, without any apparent signs of major tidal disruption or interaction with other galaxies.
