The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light distribution appears relatively even, with a gradient decreasing radially from the core. The central region shows a yellowish hue, which may indicate an older stellar population, while the outer regions show a very faint blueish tinge. The overall shape is close to round but appears subtly flattened. There is no obvious evidence of spiral arms or a distinct disk. The overall impression is of a relatively undisturbed system, not exhibiting any indications of major mergers or strong tidal interactions. The light appears uniform and no sharp discontinuities are visible.
