The galaxy presents as a roughly elliptical shape with a somewhat smooth, diffuse appearance. There is a slight deviation from a perfectly circular form. The galaxy appears primarily smooth in morphology, with a central region exhibiting a high concentration of light. The light profile fades gradually from the core, without any prominent spiral arms or a well-defined disk structure. The color gradient suggests a mixture of stellar populations, with a general shift towards redder hues. There is some indication of possible disturbances, though it could also be internal structure.
