The galaxy presents a generally smooth, elliptical morphology with a highly concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features indicative of ongoing major mergers or tidal interactions. The galaxy exhibits a radial color gradient, transitioning from a yellowish-white core to a redder outer halo. This color difference suggests the presence of an older, more evolved stellar population in the bulge region, while the outer regions may contain a relatively younger stellar population or dust. There is faint evidence of a potential disk-like structure.
