The galaxy presents a predominantly smooth morphology with a concentrated central region. A diffuse, less defined disk structure is present, exhibiting a slight elongation. The color profile suggests a dominant population of older stars, with bluer tones concentrated in the center and a redder distribution in the outer regions. There is no discernible spiral arm structure. The galaxy is relatively compact and has a moderate amount of star formation. The overall appearance suggests a low probability of undergoing any major merger activity.