The galaxy appears as a relatively compact, elliptical-like structure. Its morphology is predominantly smooth with a high degree of roundness. There are no distinct spiral arms or a well-defined disk component visible in this image. The galaxy exhibits an overall yellowish-red hue, suggesting an older stellar population. There are small, less pronounced disturbed features. The object does not present with significant signs of active merging, though there are some signs that it may be interacting with another object.
