The galaxy presents a generally smooth and elliptical morphology. It exhibits a bright, concentrated central bulge which appears roughly spherical. The galaxy displays a color gradient, appearing more yellow-orange in the core, possibly indicative of an older stellar population. The outer regions of the galaxy fade gradually, exhibiting a slightly bluer hue compared to the core, possibly due to the presence of younger stars. There are no readily apparent spiral arms or distinct dust lanes visible. The galaxy's overall structure suggests a relatively evolved system. Based on its structure, there is little evidence of any ongoing major merger activity or significant tidal disturbances. It appears to be a fairly isolated system.
