The galaxy presents as a fairly smooth, elliptical or lenticular structure with a high degree of central concentration. It exhibits a relatively featureless morphology, lacking prominent spiral arms or distinct bar structures. The overall shape is somewhere between round and slightly elongated. There is a suggestion of minor disturbances, as the outer edges are not perfectly smooth. The galaxy displays a subtle color gradient, with a slightly bluer hue towards the center, potentially indicating younger stellar populations and some ongoing star formation activity in this region. The general smoothness and lack of well-defined spiral arms suggests a relatively evolved system with a mass on the lower end. There are no signs of any major mergers, and the galaxy appears to be relatively isolated.
