The galaxy presents as a slightly elongated, elliptical structure with a dominant central bulge. The light profile appears relatively smooth, with a concentrated core and a gradual fading towards the outer regions. There is a subtle color gradient, transitioning from a yellowish-white core to a slightly redder halo. Faint hints of a disk-like feature might be present, viewed at an oblique angle, but these are not well-defined. No prominent spiral arms or dust lanes are discernible within the galaxy's structure. There is no obvious sign of on-going or past major merger events. Any star formation within the galaxy, if present, is likely minimal.
