The galaxy appears as a somewhat rounded, luminous structure. It exhibits a largely smooth morphology, with a bright central region that gradually diffuses outwards. The color is generally yellowish-white, suggesting a population of older stars. There is little evidence of distinct spiral arms or significant dust lanes. The overall impression is of an elliptical or lenticular galaxy with a relatively quiescent stellar formation rate. Based on the observed color and morphology, the galaxy is likely to be relatively massive.
