The galaxy appears to be an elliptical galaxy due to its smooth and featureless morphology. It has a concentrated core that gradually fades to a diffuse outer region. There is no evidence of spiral arms or a prominent disk. The galaxy displays a yellowish hue, suggesting a stellar population dominated by older, redder stars and a relatively low rate of on-going star formation. The shape is somewhat elongated, indicating a non-spherical structure, possibly closer to a cigar-shaped morphology. There is a subtle suggestion of a minor disturbance in the outer regions, but no major signs of an ongoing merger event, though a past minor interaction cannot be excluded. 
