The galaxy presents a diffuse, elliptical morphology. Its color profile indicates a higher concentration of older stellar populations, appearing reddish-gold in the image. The overall light distribution is smooth, with no prominent spiral arms or distinct features immediately apparent. The galaxy appears relatively isolated, showing no strong indications of ongoing major mergers or tidal disturbances, though there might be a minor disturbance in the form of a second dimmer galaxy nearby. The galaxy appears to be mostly spheroidal, with an intermediate degree of roundness.
