The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. It exhibits a yellowish-orange hue, suggesting a population of older stars and a lower rate of ongoing star formation. The overall shape is generally round, lacking any obvious spiral arms or bar structures. There is little evidence of significant dust lanes or prominent star-forming regions within the galaxy. No major merging or tidal disturbances are readily apparent. The galaxy's smooth and rounded appearance implies a state of relative quiescence and an evolved stellar population.
