The galaxy appears to be a relatively smooth, round, and moderately sized object with a concentrated central bulge. It exhibits a color gradient, transitioning from a bluer core to redder outer regions, suggesting possible variations in stellar populations or dust content. There's no clear evidence of spiral arms or a well-defined disk, though faint features suggestive of a disturbed morphology or minor tidal interactions may be present. It does not appear to be undergoing any major merger events.
