The galaxy appears as a generally smooth object with a notable disk-like structure. It presents with a partially resolved morphology, appearing neither perfectly elliptical nor fully spiral. Its intermediate roundness suggests a classification between a spherical and a highly flattened shape. Color gradients indicate a differential distribution of stellar populations, with a central region exhibiting a reddish hue that suggests older stars. Surrounding the core, there is a subtle greenish tint, possibly indicating ongoing star formation or a younger stellar population. There are no prominent spiral arms or significant dust lanes visible, suggesting a relatively quiescent state. The galaxy exhibits no significant signs of major interactions or disturbances. Subtle color asymmetries might suggest a minor interaction, but otherwise, the object appears relatively isolated and undisturbed.
