The galaxy exhibits a relatively compact structure. Its morphology appears predominantly smooth with a notable absence of prominent spiral arms or a well-defined disk. There is a suggestion of faint, diffuse features that may indicate some level of disturbance, potentially from a minor interaction or past merger event. The primary body of the galaxy presents a gradual decrease in luminosity from its center outwards. However, there are noticeable asymmetries in its distribution suggesting a complex internal structure. The color profile is also inhomogeneous, varying across the galaxy.