The galaxy presents a predominantly smooth morphology, appearing largely featureless in this image. Its overall shape is elliptical or lenticular, exhibiting a relatively high degree of roundness, though a slight elongation is subtly present. A central bulge is visible, brighter and more concentrated, surrounded by a diffuse halo. The color gradient suggests a stellar population dominated by older stars within the bulge, with a transition to slightly younger populations in the outer regions. There is a potential hint of minor tidal disturbance or interaction, which is not clear. The system appears relatively quiescent in terms of star formation activity. There is the appearance of a potential merger in progress. 
