The galaxy presents a predominantly smooth morphology, with a hint of disk-like features. The central region exhibits a bright, concentrated bulge, transitioning into a more diffuse outer region. The galaxy appears to be elliptical with a slight elongation, not perfectly spherical but also not highly flattened. There is no visible evidence of ongoing major merging events, although some minor disturbances cannot be ruled out. The overall color profile indicates a moderate amount of star formation, but it is not dominated by young, blue stars. The redder hue suggests a population of older stars is more prevalent. There is a possibility of ongoing star formation within the disk, but it doesn't appear to be a starburst galaxy. 
