The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a fairly uniform stellar population, leaning towards older stars, indicated by the reddish-yellow hue. There is little evidence of spiral arms or significant dust lanes. The overall form exhibits high degree of roundness. There seems to be no evidence of any ongoing major mergers or significant tidal disturbances from nearby galaxies. There might be very minor disturbances, but for the most part, the galaxy appears relaxed.
