The galaxy presents a generally elliptical morphology, appearing mostly smooth with a concentrated central bulge. The galaxy exhibits a radial color gradient; the core is a yellowish-orange, suggesting an older stellar population and possibly minimal current star formation, while the outer regions show hints of bluer colors, possibly indicating some younger stars. There is no clear evidence of spiral arms or a well-defined disk structure. The overall structure appears undisturbed, with no major signs of tidal interactions or ongoing mergers. The galaxy presents as an isolated system.
