This galaxy exhibits a generally smooth morphology, appearing largely undisturbed. The central region displays a higher concentration of light, suggesting the presence of a prominent galactic nucleus. The overall shape is somewhat elliptical, showing a moderate deviation from a perfectly circular form. There is a suggestion of a faint disk-like structure. The color profile is dominated by redder hues, indicating a population of older stars and a relatively low rate of on-going star formation. There is a slight chance that there may be some minor disturbances happening. 
