The galaxy presents as a relatively smooth, concentrated object. Its overall shape is elliptical, with a high degree of symmetry and no discernible spiral arm structures or bar. The galaxy displays a gradient in color, transitioning from a yellowish-orange center to a slightly bluer outer region. This suggests a possible variation in stellar populations, with older, redder stars concentrated towards the core and potentially younger, bluer stars contributing to the outer regions, however, recent star formation is relatively low. The general lack of prominent features and high degree of central concentration imply an evolved system, with evidence of ongoing or recent merging events being minimal. The physical extent of the galaxy is rather small.