The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology with a high degree of roundness. The luminosity profile suggests a lack of distinct spiral arm structures or prominent disk features. There is no visible evidence of ongoing major merging events or significant tidal disturbances. Color gradients indicate a possible population of older stars. Star formation is likely occurring at a low rate. Overall, the galaxy appears to be a quiescent system.
