The galaxy presents as a relatively smooth, elliptical structure. Its color profile suggests a population of older stars, exhibiting a reddish-yellow hue across its core and extending outwards. There is a slight elongation, deviating marginally from a perfectly circular shape. No prominent spiral arms or distinct dust lanes are visible. There might be some hints of tidal disturbances or interactions, but these are subtle. The galaxy is relatively compact. There are no obvious signs of active star formation regions within the galaxy's visible structure.