The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology with a high degree of central concentration. The central region is characterized by a bright, yellowish-white core, indicating a population of older stars. Moving outward from the core, the color gradually shifts towards bluer hues, suggesting the presence of a younger stellar population.

There are no distinct spiral arms or a prominent disk structure visible. However, there are some slight irregularities in the outer regions that may indicate minor gravitational disturbances or interactions. The galaxy's overall shape is close to round.
