The galaxy presents a somewhat amorphous appearance, with an overall elliptical shape but lacking a clearly defined structure like spiral arms. The light distribution is not entirely uniform. A smooth, diffuse glow suggests a significant population of older stars. There is a suggestion of a disk, but it is not well defined. The galaxy displays color variations, with a concentration of redder hues indicating regions of older stellar populations or dust obscuration. Conversely, bluer areas suggest regions of more recent star formation. There is an indication of a minor disturbance, possibly an interaction with another galaxy. Overall, the galaxy's morphology appears to be somewhere between a smooth elliptical and a disturbed disk galaxy, suggesting a potentially ongoing merger event or a post-merger relaxation phase.
