The galaxy presents a mostly smooth morphology, with a high degree of central concentration. The object exhibits a generally elliptical shape, appearing somewhat elongated, but predominantly situated within a range of round to slightly oblong. There are no clear signs of spiral arm structures or a distinct disk component visible in the imagery. The primary color of the galaxy is a yellow-white hue, suggesting a dominant population of older stars. There is an area that is slightly more red-shifted to one side of the galaxy. It does not show clear evidence of ongoing major merging activity, although there may be subtle indications of minor disturbances in its overall structure. The galaxy appears to be a fairly massive system. A relatively low star formation rate is inferred from the color distribution.