The observed galaxy presents an elliptical morphology, exhibiting a centrally concentrated brightness profile that diminishes radially. The core is luminous and appears yellowish-white. The surrounding halo appears more diffuse, with a slight elongation and a mottling of color, indicating possible variations in stellar populations. There are some possible disturbances that could indicate a minor merger. The overall color index suggests a population dominated by older stars, though some indications of bluer regions are also present, potentially indicating regions of recent star formation. The galaxy is well-defined, with no obvious signs of strong tidal interactions or significant morphological disruption apart from possible signs of a minor merger.
