The galaxy appears to be of moderate size, exhibiting a somewhat elliptical shape. It presents a largely smooth morphology with a central concentration of light, suggesting a dominant bulge component. However, there are subtle features suggestive of a disk, or perhaps spiral arms, though these are not well-defined. There is evidence of some distortion, indicating possible interaction or disturbance. These disturbances appear to be relatively minor. There is a wide range of wavelengths visible in the image, from redder to bluer light, suggesting a heterogeneous stellar population.