The galaxy presents an overall elliptical morphology, appearing largely smooth and spheroidal. It exhibits a dominant, concentrated central bulge. The light distribution suggests a high degree of central concentration, typical of early-type galaxies.

The galaxy's color profile indicates a relatively evolved stellar population, with a yellowish-orange hue dominating the central region, suggesting older, cooler stars. There is a slight indication of reddish tones towards one side of the galaxy, which might suggest some dust obscuration or the presence of a small population of younger stars in that region, although the overall color suggests this is not a region of active star formation. The outer regions of the galaxy seem to be bluer than the core.

There are potential signs of tidal interactions or past mergers, with faint asymmetric features or subtle disturbances visible in the galaxy's periphery. However, these features are not particularly prominent, suggesting a relatively quiescent merger history or a system in the later stages of relaxation following a merger event.
